Twin Impact Lunar Telescope network: Lunar Impact Flash observations of the 2025 Geminids

Aldo Tonon; Alex Pratt; Andrea Ferrero; Anthony Cook; Bruno Mongellaz; Chris Hooker; Christelle Saliby; Chrysa Avdellidou; Daniel Sheward; Detlef Koschny

REVIEW 5 major objections 3 minor 298 references

Twin Impact Lunar Telescope network: Lunar Impact Flash observations of the 2025 Geminids

T0 review · 5 major / 3 minor · reviewed 2026-08-03 · deepseek-v4-flash

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Pith's one-line read During the 2025 Geminids, a single automated telescope station detected 53 candidate lunar impact flashes and confirmed 11 as genuine impacts, with magnitudes between +7.5 and +10.4 — enough to validate the station and to argue that even un

desk verdict First TILT1 Geminid dataset is a genuinely useful proof-of-concept, but the '11 confirmed' headline rests partly on private communications and an internal inconsistency that should be fixed before the counting claims are taken at face value. read the letter →

arxiv 2607.29481 v1 pith:DL5HX6RZ submitted 2026-07-31 astro-ph.EP astro-ph.IM

Daniel Sheward , Marco Delbo , Chrysa Avdellidou , Philippe Lognonné , Jeremie Vaubaillon , Pierre-Yves Froissart , Christelle Saliby , Paul Girard

show 18 more authors

Nicolas Mauclert Bruno Mongellaz Laurent Herrier Nicolas Anfosso Thierry Parra Fausto Giacometti Andrea Ferrero Jean-Pierre Rivet Elisa Maria Alessi Anthony Cook Detlef Koschny James Dawson Chris Hooker Alex Pratt Michael O'Connell Aldo Tonon Vincenzo della Vecchia Luigi Zanatta

This is my paper · ORCID

classification astro-ph.EPastro-ph.IM

keywords lunarimpactflashesGeminidsmeteoroidstreamimpactsseismologymulti-messengerobservationtelescopenetworkflashdetectionCMOShigh-speedimaging

verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper reports the first observing campaign of a newly built automated telescope station designed to watch the Moon for impact flashes. Over the two peak nights of the 2025 Geminid meteor shower, it captured 53 candidate flashes and confirmed 11 as genuine lunar impacts, with magnitudes +7.5 to +10.4. The authors argue this rate — about 1.3 confirmed flashes per hour — shows the station works and that high-ZHR streams are ideal for such observations. Their central forward-looking claim is that even flashes seen by only one telescope, without independent confirmation, can still be scientifically useful: when future seismometers on the Moon detect an impact-generated seismic signal, the optical flash's time and location can be matched to it, turning single-station telescopes into participants in lunar interior studies.

What carries the argument

The carrying instrument is the TILT1 station: two co-aligned 400-mm telescopes (one near-infrared, one visible-light camera during the campaign) operated at 50-ms exposures with continuous lunar tracking, plus detection software that flags 5-sigma brightness transients. Confirmation of flashes relies on two independent routes — persistence across multiple frames and matching detections by other observers. The paper's conceptual machinery is the pairing of a flash's measured time and lunar coordinates with a future seismometer record: the flash pins the seismic source's location and time, leaving only the interior's seismic propagation properties as unknowns.

What would settle it

For each of the five 'confirmed via private communication' events, look for a public record of the same flash at the same time in any published lunar impact archive; if none exist, the eleven-event confirmation count and the derived detection rate rest on unverifiable testimony. Additionally, re-examine the six two-frame events to see whether moving satellites or electronic artefacts could mimic a brief flash in consecutive frames.

Watch

Extended reading notes

Core claim

On 13–14 December 2025, the first station of the TILT network — a twin 40-cm telescope system — observed the Moon at about 20 frames per second and detected 53 candidate impact flashes above 5-sigma. Eleven were confirmed: six appeared in at least two frames and five were independently seen by other observers. These confirmed flashes span magnitude +7.5 to +10.4 and correspond to sub-kilogram meteoroids, mostly tied to the Geminid stream. The paper argues that the unconfirmed single-frame flashes cannot all be dismissed as false positives: their magnitude distribution and the elevated candidate rate suggest some are real impacts. Its central multi-messenger claim is that an optical flash — c

Load-bearing premise

The headline count of eleven confirmed lunar impacts depends on five events that are confirmed only by private communications from other observers (with no public times, images, or station data) and on six events that appeared in only two frames without the point-spread-function check that could reject non-astronomical artefacts.

Editorial extensions

If this is right

A single automated station can sustain a LIF detection rate of about 1.3 confirmed flashes per hour during a strong meteor shower, comparable to previous dedicated campaigns.
Unconfirmed single-station flashes should not be discarded; they can be archived and later matched to seismic signals from the Moon, effectively confirming them retroactively.
High-ZHR streams such as the Geminids are prime targets for LIF monitoring, and a global network of stations would maximize coverage of rare, more energetic impacts.
The detected impactor masses (tens to hundreds of grams) are within the detection range of upcoming seismometers within tens of kilometres, so optical-seismic coincidence is feasible.
A network of three such stations would provide continuous dark-side lunar monitoring, increasing the chance of catching the larger impacts most useful for seismology.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

If the field adopted a shared public registry of single-station flash candidates, amateur and professional observers alike could contribute to seismic source localization without needing expensive multi-station setups.
The paper's confirmation of five events through private communication rather than public data suggests that a public timestamped reporting culture would strengthen the evidentiary basis for future impact flash surveys.
A PSF-shape rejection step, which the paper did not perform, could filter out cosmic-ray and electronic artefacts and likely raise the fraction of genuine flashes among the 53 candidates, making the unconfirmed pool more reliable for seismic matching.
The observed high rate of candidates relative to confirmed events implies that the timing glitch in the camera acquisition cost the survey many real detections; fixing it could substantially increase the confirmed-event rate without any change in telescope size.

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Signed reviews

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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Desk Editor's Note

read the letter

Worth a look: this is the first dataset from the TILT1 station, and the paper is refreshingly honest about the camera timing failures, unsynchronized exposures, and lost energy. The new idea—using unconfirmed single-station LIF candidates for future seismic correlation—is forward-looking and sensible, and the seismic framing is well grounded in the upcoming Chang'e-7, FSS, and SPSS missions. The authors also deserve credit for comparing their rates against NELIOTA and prior Geminid campaigns rather than overclaiming.

The soft spots are real but addressable. Five of the eleven 'confirmed' events (IDs 34, 45, 46, 49, 52) rest on private communication with A. Cook, with no public times, images, or station data. An independent reader cannot verify those. Six other confirmations are two-frame detections on a single camera, and the paper explicitly says the PSF analysis to reject non-LIF transients was not performed. Two frames on one unsynchronized detector is not airtight. And there is a genuine internal inconsistency: §4.1 lists IDs 10, 24, and 34 as multi-frame events, but Table A1 lists Frames=1 for all three. That needs to be corrected, and it suggests the event classification should be carefully rechecked.

Photometry is another place to be cautious. Unfiltered CMOS with assumed κ=0.25, f=2, and Δλ=0.3 μm, plus ±0.1 mag errors that omit systematics, makes the energy and mass columns rough estimates. The interpolated readout energy is honestly labeled a 'best-guess,' so I would not build quantitative conclusions on those numbers. The rate comparison is also handled inconsistently: the abstract says 'high rate,' but the body shows the confirmed rate of 1.3±0.3 h−1 is lower than Yanagisawa et al.'s 2.6±0.28 h−1. The 'high rate' only holds for candidates, and the authors know it.

The seismic coupling model is tuned with a linear factor and an extrapolated attenuation; that is stated as empirical, so it is a minor concern. The circularity burden is low: η from Sheward et al. (2025) is an external calibration and does not affect whether flashes were detected.

Bottom line: the central claim—that TILT1 detected real LIFs and can operate as an autonomous station—is plausible, but the evidence as presented is not fully auditable. This deserves peer review, not desk rejection, but the authors should be asked to release the confirming observers' data, perform or explicitly justify skipping PSF analysis, fix the frame-count inconsistency, and present dead-time-corrected rates. I would not cite it in its current form, but I would read a revised version.

Referee Report

5 major / 3 minor

Summary. During the 2025 Geminids maximum, the first TILT station observed the Moon for 8.5 hours with three unfiltered cameras. The paper reports 53 candidate flashes, of which 11 are claimed as confirmed (six multi-frame events and five matched through private communication with the LUMIO campaign coordinator). For all events the paper derives magnitudes, luminous and kinetic energies, stream association probabilities, and masses, and compares observed rates with NELIOTA and previous Geminid campaigns. It further argues that even unconfirmed single-station candidates will be useful as targets for correlation with future lunar seismometers.

Significance. The paper's main value is proof-of-concept: a modest-aperture autonomous station can detect a large number of LIF candidates during a high-ZHR stream, and the proposed use of candidate events as seismic correlation targets is a sensible path for future multi-messenger lunar science. The manuscript is commendably explicit about the acquisition timing problem and about the fact that PSF analysis was not performed. However, the central quantitative claims — the '11 confirmed' events, the associated 1.3±0.3 h^-1 rate, and the energy/mass entries in Table A1 — depend on confirmation criteria that are not fully auditable. The paper's own text contains a contradiction between §4.1 and Table A1 regarding three multi-frame events. With access to the underlying event data these issues can be resolved; without such data the headline statistics are not reproducible.

major comments (5)

[§4.1, Table A1] The text states that the multi-frame events ID 10, 24, and 34 had readout times longer than 50 ms and 'would have been at least three frames long' if exposures had been saved correctly, yet Table A1 lists Frames=1 for all three. If these are intended to be among the six multi-frame confirmations, the confirmed-event count is internally inconsistent; if not, the passage should be corrected. Please reconcile the text and table and give per-event frame counts and readout intervals.
[§4.1, §5; Table A1] The six events counted as confirmed because they appear in two consecutive frames (IDs 11, 17, 18, 25, 35, 42) are not corroborated by a second synchronized camera, and the paper explicitly states that the PSF analysis 'is not performed here' (§5). With variable frame delays of tens to hundreds of ms and unsynchronized cameras, a two-frame transient in one detector is not sufficient as presented to exclude satellite glints or detector artifacts. Please provide PSF analysis, thumbnails, or light curves for these six events, or reclassify them as candidates and adjust the headline '11 confirmed' and the rate 1.3±0.3 h^-1 accordingly.
[§4.1, Table A1 (IDs 34, 45, 46, 49, 52)] Five 'confirmed' events rest on private communication with A. Cook; no public times, images, or station data are given. Because the table reports only TILT1's own measurements for these IDs, an independent reader cannot verify that a second observer exists. Please include the external confirmation data (observer, station, time, magnitude, or public event identification) or mark these as unconfirmed and recompute the confirmed-event statistics.
[§4.2, Eq. (5)] The adopted luminous efficiency η=6.0±1.2×10^-3 from Sheward et al. (2025) lies outside the range 5×10^-4 to 1.5×10^-3 quoted in the same paragraph. Since E_k and all derived masses scale as 1/η, the Table A1 masses and the seismic-detectability discussion depend strongly on this choice. Please justify the adopted value for unfiltered visible+NIR observations, propagate its uncertainty, and discuss the resulting systematic range.
[§4.1, Eqs. (1)–(4)] The luminous energy calculation uses assumed values κ=0.25 mag/airmass, f=2, and Δλ=0.3 μm without uncertainties, while the unfiltered camera response extends to ~1000 nm. The quoted ±0.1 mag errors are statistical only and do not include these systematics, so the E_k and mass uncertainties in Table A1 are understated. Please add a systematic error budget or explicitly state that the derived masses are order-of-magnitude estimates.

minor comments (3)

[Figure 4 caption] 'Impulse have been computed' should read 'Impulses have been computed'.
[§4.1, Table A1] The 'Mag' column is labeled 'Peak' but the passband is not stated; since observations were unfiltered, specify the effective wavelength/band or state that the magnitudes are clear-filter estimates.
[Data Availability] The statement that data are 'available upon email request' is insufficient for confirmation-based claims. Please deposit event lists, light curves, and external confirmation records in a public archive.

Circularity Check

0 steps flagged · score 0.0 of 10

No circularity found: flash detection is observational, energy/mass scaling uses external calibrations, and the seismic range model is explicitly empirical.

full rationale

The derivation chain is not circular. The central claim—53 candidates and 11 confirmed flashes—is an observational classification from image sequences and external observer reports; it is not the output of any fitted model, and Equations (1)–(4) are standard photometric and luminous-energy conversions calibrated against transiting stars. The luminous efficiency η=6.0×10^-3 (Sheward et al. 2025) is a self-citation, but it is an external crater-calibrated value that does not feed back into flash detection, confirmation, or photometry; if it were in error only the inferred masses/energies would change, not the detection claim. The seismic-detection model explicitly tunes a linear coupling factor to reproduce the Apollo rate of 68 impacts/yr and is labelled empirical, so it is a calibration, not a prediction masquerading as independent. The paper itself flags the main limitations: cameras were unsynchronized, no PSF analysis was performed ('this step is not performed here'), and five confirmations rest on private communication with A. Cook. These are verification weaknesses—and there is an internal inconsistency in §4.1 listing IDs 10, 24, 34 as multi-frame while Table A1 lists Frames=1—but none of them make the derivation circular. No uniqueness theorem, ansatz, or renaming from the authors' prior work is used to force the conclusions.

Assumptions & free parameters 6 free parameters · 6 assumptions · 0 invented entities

No new physical entities are postulated. The paper's derived quantities rest on assumed photometric parameters (κ, f, Δλ, η), on unverifiable private confirmations, and on an empirically tuned seismic model; those are the main free inputs, not new particles or forces.

free parameters (6)

Extinction coefficient κ = 0.25 mag/airmass
Assumed constant for calibrating transiting stars at different airmasses (Eq. 1); no site-specific extinction measurement; systematic errors enter all magnitudes and luminosities.
Isotropy factor f = 2
Assumed flash radiates into a hemisphere (Eq. 4); factor-of-2 uncertainty in E_lum.
Wavelength band Δλ = 0.3 μm
Unfiltered CMOS cameras; adopted V/R bandwidth; actual response extends to 1000 nm, biasing E_lum.
Luminous efficiency η = 6.0±1.2×10⁻³
Taken from Sheward et al. (2025), same group; the older literature range spans 5×10⁻⁴ to 1.5×10⁻³; all reported masses scale as 1/η.
Seismic linear coupling factor = not stated numerically
Tuned in §5 ('by tuning the linear coupling factor...') to reproduce the Apollo rate of 68 impacts/year in the seismic detectability model.
Attenuation extrapolation ratio q(5Hz)/q(0.5Hz) = 10
Ad hoc extrapolation from 0.5 Hz to 5 Hz for the seismic amplitude–distance model in §5.

assumptions (6)

domain assumption Human vetting plus a 5σ threshold is sufficient to identify LIF candidates without PSF analysis
Stated in §5: the PSF analysis step 'is not performed here'; cosmic-ray/satellite rejection relies on visual inspection.
domain assumption Multi-frame events are genuine LIFs
Table A1 caption says 'Events with multiple frames are confirmed LIFs'; no PSF or spectral confirmation is provided.
ad hoc to paper Private communications via A. Cook are reliable independent confirmations
Five events († IDs 34, 45, 46, 49, 52) are confirmed by other observers; no public data, times, or station details are given.
domain assumption Unfiltered camera measurements can be calibrated with V/R stellar photometry and an assumed extinction coefficient
Photometry in §4.1; unfiltered response extends beyond R band, so color terms are ignored.
domain assumption The stream-association probability method of Avdellidou et al. (2021) correctly assigns Geminid vs sporadic origin
Used for impact velocity and mass; Geminid probabilities have a median of 89% and a minimum of 61%; the method is cited, not re-derived.
domain assumption The seismic detectability model calibrated on Apollo SIV-B impacts applies to future instruments
§5 extrapolates from 0.5 Hz to 5 Hz with a q-factor and a tuned coupling; the authors call the model 'empirical'.

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Cite this review

Pith. "Pith review of Twin Impact Lunar Telescope network: Lunar Impact Flash observations of the 2025 Geminids." pith.science (2026). https://pith.science/paper/DL5HX6RZ

@misc{pith2026260729481,
  author       = {Pith},
  title        = {Pith review of: Twin Impact Lunar Telescope network: Lunar Impact Flash observations of the 2025 Geminids},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/DL5HX6RZ}},
  note         = {Machine review of arXiv:2607.29481}
}

read the original abstract

Meteoroid impacts on the Moon, observed from Earth as flashes typically lasting a few tens of milliseconds, have been monitored for three decades for determining meteoroids' size and mass frequency distribution in the cm to dm range. Studies link these observed impact events to fresh craters advancing our understanding of energy partitioning during an impact. Currently we are transitioning to a new era where lunar impact flashes (LIFs) can be used to supplement upcoming lunar seismology to study the internal lunar structure. Here we present results from the first station of a telescope network under development for continuous LIF monitoring. Observations were carried out during the Geminids 2025 campaign, initiated by the LUMIO Science Team in the framework of their public engagement activities. We detected 53 potential impact flashes and confirmed 11 of them through multiframe observations, and independent detections by other observers. We present evidence suggesting that some of the yet unconfirmed events may be real. Our confirmed events range between magnitude +7.5 and +10.4, primarily in the V and R band. We obtained a high rate of observations per hour, highlighting the importance of high ZHR meteoroid streams for observing LIFs. We also discuss the scientific value of potential LIFs that remain unconfirmed in optical data alone. Even without multi station confirmation, these events can correlate to seismic signals in future lunar seismic networks, thereby providing useful physical constraints on impact processes. This approach would also allow stations equipped with a single telescope/camera to meaningfully contribute to the network.

Figures

Figures reproduced from arXiv: 2607.29481 by the authors.

**Figure 2.** Magnitude decay curves for each of the six observed multi-frame events. While each event shown is only two frames long, the difference in duration is due to the computing issue, which caused large delays during readout times, or lost frames. 10, 24, and 34) each had a readout times longer than 50 msec, and thus would have been at least three frames long had the camera software correctly saved the exposures. The var… view at source ↗

**Figure 3.** Relative cumulative frequency densities for confirmed LIF observations (green), and all event observations (orange), compared to that of the NELIOTA campaigns confirmed LIF observations (black). impacts occur at a much lower frequency, maximising observational time for the purposes of catching these ’lucky’ events is crucial. A network of multiple observing stations distributed across the globe would therefore allo… view at source ↗

**Figure 4.** Comparison of the masses of the Geminid detected LIFs with the detection range of Apollo SP, Chang’e-7 broad-band, and the VBBZ instrument onboard FSS and SPSS. Impulse have been computed assuming a 20 km s−1 velocity impacting at 45°. impactors mass-frequency distribution as proposed by Brown et al. (2002), that the impact velocities are 20 km s−1 impacting at 45°, and that the distance dependency is the one calibr… view at source ↗

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Works this paper leans on

298 extracted references · 93 canonical work pages

[1]

JPL , year = 2016, url =

2016
[2]

AIDA Study , year = 2016, url =

2016
[3]

DAWN mission , year = 2016, url =

2016
[4]

Asteroid Physical Properties, ESA , year = 2017, url =

2017
[5]

Ruff Database , year = 2016, url =

2016
[6]

Asteroids III, W

Meteoritic Parent Bodies: Their Number and Identification. Asteroids III, W. F. Bottke Jr., A. Cellino, P. Paolicchi, and R. P. Binzel (eds), University of Arizona Press, Tucson, p.653-667 , year = 2002, editor =

2002
[7]

Asteroids IV , year = 2015, editor =

Astronomical Observations of Volatiles on Asteroids. Asteroids IV , year = 2015, editor =. doi:10.2458/azu_uapress_9780816532131-ch004 , adsurl =

work page doi:10.2458/azu_uapress_9780816532131-ch004 2015
[8]

doi:10.1007/978-1-4419-0324-2 , adsurl =

Lunar Meteoroid Impacts and How to Observe Them. doi:10.1007/978-1-4419-0324-2 , adsurl =

work page doi:10.1007/978-1-4419-0324-2

Show all 298 references

[9]

Asteroids III , year = 2002, editor =

Mineralogy of Asteroids. Asteroids III , year = 2002, editor =

2002
[10]

Los Alamos series on dynamic material properties , publisher =
[11]

Meteorites and the Early Solar System II , year = 2006, editor =

Systematics and Evaluation of Meteorite Classification. Meteorites and the Early Solar System II , year = 2006, editor =

2006
[12]

Meteorites and the Early Solar System II , year = 2006, editor =

Types of extraterrestrial material available for study. Meteorites and the Early Solar System II , year = 2006, editor =

2006
[13]

Meteor Showers and their Parent Comets
[14]

Comets II , year = 2004, editor =

Structure and density of cometary nuclei. Comets II , year = 2004, editor =

2004
[15]

ArXiv e-prints , keywords =

The Compositional Structure of the Asteroid Belt. ArXiv e-prints , keywords =
[16]

Asteroids IV , editor =

Asteroid impacts and modern civilisation: Can we prevent a catastrophe?. Asteroids IV , editor =
[17]

Asteroids IV , editor =

Cratering on Asteroids. Asteroids IV , editor =
[18]

The Exoplanet Handbook, by Michael Perryman, Cambridge, UK: Cambridge University Press, 2014 , year = 2014, month = jan, adsurl =

The Exoplanet Handbook. The Exoplanet Handbook, by Michael Perryman, Cambridge, UK: Cambridge University Press, 2014 , year = 2014, month = jan, adsurl =

2014
[19]

Asteroids , year = 1979, editor =

Collisional evolution of asteroids - Populations, rotations, and velocities. Asteroids , year = 1979, editor =

1979
[20]

Comets II , year = 2004, editor =

The sizes, shapes, albedos, and colors of cometary nuclei. Comets II , year = 2004, editor =

2004
[21]

The Solar System Beyond Neptune , year = 2008, editor =

Colors of Centaurs. The Solar System Beyond Neptune , year = 2008, editor =

2008
[22]

Icarus , year = 1999, month = jan, volume = 137, pages =

The Missing Psyche Family: Collisionally Eroded or Never Formed?. Icarus , year = 1999, month = jan, volume = 137, pages =. doi:10.1006/icar.1998.6037 , adsurl =

1999
[23]

The Solar System Beyond Neptune , year = 2008, editor =

The Early Development of Ideas Concerning the Transneptunian Region. The Solar System Beyond Neptune , year = 2008, editor =

2008
[24]

The Solar System Beyond Neptune , year = 2008, editor =

Color Properties and Trends of the Transneptunian Objects. The Solar System Beyond Neptune , year = 2008, editor =

2008
[25]

The Solar System Beyond Neptune , year = 2008, editor =

On the Atmospheres of Objects in the Kuiper Belt. The Solar System Beyond Neptune , year = 2008, editor =

2008
[26]

The Solar System Beyond Neptune , year = 2008, editor =

The Structure of Kuiper Belt Bodies: Link with Comets. The Solar System Beyond Neptune , year = 2008, editor =

2008
[27]

ArXiv e-prints , archivePrefix = "arXiv", eprint =

New Paradigms For Asteroid Formation. ArXiv e-prints , archivePrefix = "arXiv", eprint =
[28]

Comets II , year = 2004, editor =

Oort cloud formation and dynamics. Comets II , year = 2004, editor =

2004
[29]

Asteroids II , year = 1989, editor =

Asteroid taxonomic classifications. Asteroids II , year = 1989, editor =

1989
[30]

Comets II , year = 2004, editor =

The Kuiper belt and the primordial evolution of the solar system. Comets II , year = 2004, editor =

2004
[31]

Compositional structure in the asteroid belt: Results of a spectroscopic survey
[32]

Asteroids IV , year = 2015, pages =

Cratering on Asteroids. Asteroids IV , year = 2015, pages =. doi:10.2458/azu_uapress_9780816532131-ch037 , adsurl =

2015 doi
[33]

Asteroids, Comets, Meteors 2014 , year = 2014, editor =

Porosity as a significant factor for asteroid survival. Asteroids, Comets, Meteors 2014 , year = 2014, editor =

2014
[34]

Lunar and Planetary Science Conference , year = 2016, series =

Analysis of Lunar Impact Flashes Recorded During the Activity Period of the Lyrid Meteor Shower in 2013. Lunar and Planetary Science Conference , year = 2016, series =

2013
[35]

Lunar and Planetary Science Conference , year = 1998, series =

Light Impulse Created by Meteoroids Impacting the Moon. Lunar and Planetary Science Conference , year = 1998, series =

1998
[36]

EPSC-DPS Joint Meeting 2019 , year = 2019, volume =

PyNAPLE: Automated Lunar Impact Flash Crater Detection. EPSC-DPS Joint Meeting 2019 , year = 2019, volume =

2019
[37]

EPSC-DPS Joint Meeting 2019 , year = 2019, volume =

Automating the detection and coordinate identification of impact flashes on the Lunar surface. EPSC-DPS Joint Meeting 2019 , year = 2019, volume =

2019
[38]

, keywords =

New crater on the Moon and a swarm of secondaries. , keywords =. doi:10.1016/j.icarus.2015.01.019 , adsurl =

2015 doi
[39]

, keywords =

NELIOTA: The wide-field, high-cadence, lunar monitoring system at the prime focus of the Kryoneri telescope. , keywords =. doi:10.1051/0004-6361/201833499 , archivePrefix =. 1809.00495 , primaryClass =

arXiv
[40]

VizieR Online Data Catalog , keywords =

VizieR Online Data Catalog: Precession Formulae and Mean Elements for Moon and Planets (Simon+ 1994). VizieR Online Data Catalog , keywords =

1994
[41]

, year = 1965, month = sep, volume =

Topography of the Moon. , year = 1965, month = sep, volume =. doi:10.1007/BF00216275 , adsurl =

1965 doi
[42]

, keywords =

Debiased albedo distribution for Near Earth Objects. , keywords =. doi:10.1016/j.icarus.2020.113631 , archivePrefix =. 2001.03550 , primaryClass =

2020
[43]

, keywords =

The cratering history of asteroid (21) Lutetia. , keywords =. doi:10.1016/j.pss.2011.10.010 , archivePrefix =. 1111.3628 , primaryClass =

2011 arXiv
[44]

, keywords =

Craters on comets. , keywords =. doi:10.1016/j.pss.2014.06.008 , adsurl =

2014 doi
[45]

Scientific American , year = 1949, month = jul, volume =

The Craters of the Moon. Scientific American , year = 1949, month = jul, volume =. doi:10.1038/scientificamerican0749-20 , adsurl =

1949 doi
[46]

, year = 1971, month = feb, volume =

On the History of Lunar Impact Cratering: The Absolute Time Scale and the Origin of Planetesimals. , year = 1971, month = feb, volume =. doi:10.1016/0019-1035(71)90100-X , adsurl =

1971 doi
[47]

, year = 2001, month = apr, volume =

Mars/Moon Cratering Rate Ratio Estimates. , year = 2001, month = apr, volume =

2001
[49]

, year = 2001, month = apr, volume =

Cratering Records in the Inner Solar System in Relation to the Lunar Reference System. , year = 2001, month = apr, volume =

2001
[50]

, year = 2001, month = apr, volume =

Cratering Chronology and the Evolution of Mars. , year = 2001, month = apr, volume =. doi:10.1023/A:1011945222010 , adsurl =

2001 doi
[51]

, year = 2005, month = jun, volume =

Modeling crater populations on Venus and Titan. , year = 2005, month = jun, volume =. doi:10.1016/j.pss.2005.03.002 , adsurl =

2005 doi
[52]

International Journal of Impact Engineering , year = 1987, month = jan, volume =

Some recent advances in the scaling of impact and explosion cratering. International Journal of Impact Engineering , year = 1987, month = jan, volume =

1987
[53]

, keywords =

Catastrophic disruptions and cratering of solar system bodies: a review and new results. , keywords =. doi:10.1016/0032-0633(94)90007-8 , adsurl =

doi
[54]

Science , keywords =

Diviner Lunar Radiometer Observations of the LCROSS Impact. Science , keywords =. doi:10.1126/science.1197135 , adsurl =

doi
[55]

, keywords =

Hypervelocity cratering and disruption of the Northwest Africa 869 ordinary chondrite meteorite: Implications for crater production, catastrophic disruption, momentum transfer and dust production on asteroids. , keywords =. doi:10.1016/j.pss.2018.06.019 , adsurl =

2018 doi
[56]

, year = 2016, month = may, volume =

Ranger and Apollo S-IVB spacecraft impact craters. , year = 2016, month = may, volume =. doi:10.1016/j.pss.2016.01.002 , adsurl =

2016 doi
[57]

, keywords =

Hypervelocity cratering and disruption of the Northwest Africa 4502 carbonaceous chondrite meteorite: Implications for crater production, catastrophic disruption, momentum transfer and dust production on asteroids. , keywords =. doi:10.1016/j.pss.2020.104916 , adsurl =

2020
[58]

, year = 2004, month = oct, volume =

Chemical and mineralogical size segregation in the impact disruption of inhomogeneous, anhydrous meteorites. , year = 2004, month = oct, volume =. doi:10.1016/j.pss.2004.07.010 , adsurl =

2004 doi
[59]

Science , keywords =

The LCROSS Cratering Experiment. Science , keywords =. doi:10.1126/science.1187454 , adsurl =

doi
[60]

Science , keywords =

Detection of Water in the LCROSS Ejecta Plume. Science , keywords =. doi:10.1126/science.1186986 , adsurl =

doi
[61]

Nature Communications , year = 2013, month = oct, volume =

Characterization of the LCROSS impact plume from a ground-based imaging detection. Nature Communications , year = 2013, month = oct, volume =. doi:10.1038/ncomms3620 , adsurl =

2013 doi
[62]

, year = 2007, month = jan, volume =

The Deep Impact oblique impact cratering experiment. , year = 2007, month = jan, volume =. doi:10.1016/j.icarus.2007.06.031 , adsurl =

2007 doi
[63]

, year = 2013, month = feb, volume =

The Deep Impact crater on 9P/Tempel-1 from Stardust-NExT. , year = 2013, month = feb, volume =. doi:10.1016/j.icarus.2012.06.018 , adsurl =

2013 doi
[64]

, year = 2011, month = jul, volume =

Nonuniform cratering of the Moon and a revised crater chronology of the inner Solar System. , year = 2011, month = jul, volume =. doi:10.1016/j.icarus.2011.03.010 , adsurl =

2011 doi
[65]

, keywords =

Asteroid Impact & Deflection Assessment mission: Kinetic impactor. , keywords =. doi:10.1016/j.pss.2015.12.004 , adsurl =

2015 doi
[66]

Science , keywords =

An artificial impact on the asteroid (162173) Ryugu formed a crater in the gravity-dominated regime. Science , keywords =. doi:10.1126/science.aaz1701 , adsurl =

doi
[67]

Meteoritics and Planetary Science , year = 2020, month = oct, volume =

Impact flash evolution of CO _ 2 ice, water ice, and frozen Martian and lunar regolith simulant targets. Meteoritics and Planetary Science , year = 2020, month = oct, volume =. doi:10.1111/maps.13581 , adsurl =

2020 doi
[68]

, keywords =

Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O - M stars. , keywords =
[69]

WGN, Journal of the International Meteor Organization , year = 1991, month = apr, volume =

Calculating the solar longitude 2000.0. WGN, Journal of the International Meteor Organization , year = 1991, month = apr, volume =

2000
[70]

, keywords =

P/Halley dust characteristics - A comparison between Orionid and Eta Aquarid meteor observations and those from the flyby spacecraft. , keywords =
[71]

Journal of Spacecraft and Rockets , keywords =

Meteor shower forecasting in near-Earth space. Journal of Spacecraft and Rockets , keywords =. doi:10.2514/1.A34416 , archivePrefix =. 1904.06370 , primaryClass =

1904 arXiv
[72]

, keywords =

NELIOTA: Methods, statistics, and results for meteoroids impacting the Moon. , keywords =. doi:10.1051/0004-6361/201936709 , archivePrefix =. 1911.06101 , primaryClass =

1911 arXiv
[73]

Science , keywords =

Impact craters on Pluto and Charon indicate a deficit of small Kuiper belt objects. Science , keywords =. doi:10.1126/science.aap8628 , archivePrefix =. 1902.10795 , primaryClass =

1902 arXiv
[74]

AAS/Division for Planetary Sciences Meeting Abstracts , year = 2014, series =

Meteorite Source Regions as Revealed by the Near-Earth Object Population. AAS/Division for Planetary Sciences Meeting Abstracts , year = 2014, series =

2014
[75]

Meteoroids: The Smallest Solar System Bodies , year = 2011, editor =

An Exponential Luminous Efficiency Model for Hypervelocity Impact into Regolith. Meteoroids: The Smallest Solar System Bodies , year = 2011, editor =

2011
[76]

AAS/Division for Planetary Sciences Meeting Abstracts \#34 , year = 2002, series =

Near-Infrared Spectroscopy of Henan and Watsonia Family Asteroids. AAS/Division for Planetary Sciences Meeting Abstracts \#34 , year = 2002, series =

2002
[77]

Asteroids II , year = 1989, editor =

Meteoritic parent bodies - Nature, number, size and relation to present-day asteroids. Asteroids II , year = 1989, editor =

1989
[78]

37th Annual Lunar and Planetary Science Conference , year = 2006, series =

Shape, Spin, and the Structure of Asteroids, Centaurs, and Kuiper Belt Objects. 37th Annual Lunar and Planetary Science Conference , year = 2006, series =

2006
[79]

37th Annual Lunar and Planetary Science Conference , year = 2006, series =

Small Body Density and Porosity: New Data, New Insights. 37th Annual Lunar and Planetary Science Conference , year = 2006, series =

2006
[80]

Lunar and Planetary Science Conference , year = 2008, volume = 39, month = mar, pages =

Asteroids on the Moon: Projectile Survival During Low Velocity Impact. Lunar and Planetary Science Conference , year = 2008, volume = 39, month = mar, pages =

2008
[81]

Lunar and Planetary Science Conference , year = 2013, volume = 44, month = mar, pages =

Experimental Studies into the Survival and State of the Projectile. Lunar and Planetary Science Conference , year = 2013, volume = 44, month = mar, pages =

2013
[82]

Lunar and Planetary Science Conference , year = 2014, volume = 45, month = mar, pages =

How much of the Impactor (and Its Water) Ends up in Vesta's Regolith?. Lunar and Planetary Science Conference , year = 2014, volume = 45, month = mar, pages =

2014
[83]

Lunar and Planetary Science Conference , year = 2015, volume = 46, month = mar, pages =

New Constraints on the Delivery of Impactors to Icy Bodies: Implications for Ceres. Lunar and Planetary Science Conference , year = 2015, volume = 46, month = mar, pages =

2015
[84]

Lunar and Planetary Science Conference Proceedings , year = 1973, series =

Microcraters on Apollo 15 and 16 samples and corresponding cosmic dust fluxes. Lunar and Planetary Science Conference Proceedings , year = 1973, series =

1973
[85]

EPSC-DPS Joint Meeting 2019 , year = 2019, volume =

Real-time detection of impact flashes on the lunar surface. EPSC-DPS Joint Meeting 2019 , year = 2019, volume =

2019
[86]

, keywords =

Interpreting the Cratering Histories of Bennu, Ryugu, and Other Spacecraft-explored Asteroids. , keywords =. doi:10.3847/1538-3881/ab88d3 , adsurl =

doi
[87]

DellaGiustina, D. N. and Burke, K. N. and Walsh, K. J. and Smith, P. H. and Golish, D. R. and Bierhaus, E. B. and Ballouz, R.-L. and Becker, T. L. and Campins, H. and Tatsumi, E. and Yumoto, K. and Sugita, S. and Deshapriya, J. D. Prasanna and Cloutis, E. A. and Clark, B. E. a...

2020
[88]

, keywords =

Temperatures of lunar impact flashes: mass and size distribution of small impactors hitting the Moon. , keywords =. doi:10.1093/mnras/stz355 , archivePrefix =. 1902.00987 , primaryClass =

1902 arXiv
[89]

Science , year = 2020, month = oct, volume =

Bennu’s near-Earth lifetime of 1.75 million years inferred from craters on its boulders. Science , year = 2020, month = oct, volume =

2020
[90]

Nature Geoscience , year =

Walsh, K J and Jawin, E R and Ballouz, R L and Barnouin, O S and Bierhaus, E B and Connolly, H C and Molaro, J L and McCoy, T J and Delbo, M and Hartzell, C M and Pajola, M and Schwartz, S R and Trang, D and Asphaug, E and Becker, K J and Beddingfield, C B and Bennett, C A and...
[91]

Science , keywords =

The geomorphology, color, and thermal properties of Ryugu: Implications for parent-body processes. Science , keywords =. doi:10.1126/science.aaw0422 , adsurl =

doi
[92]

Earth Moon and Planets , keywords =

The NASA Lunar Impact Monitoring Program. Earth Moon and Planets , keywords =. doi:10.1007/s11038-007-9184-0 , adsurl =

doi
[93]

Earth Moon and Planets , keywords =

Algorithms for Lunar Flash Video Search, Measurement, and Archiving. Earth Moon and Planets , keywords =. doi:10.1007/s11038-007-9226-7 , adsurl =

doi
[94]

, keywords =

Identification of the SMART-1 spacecraft impact location on the Moon. , keywords =. doi:10.1016/j.icarus.2018.11.009 , adsurl =

2018 doi
[95]

, keywords =

SMART-1 technology, scientific results and heritage for future space missions. , keywords =. doi:10.1016/j.pss.2017.09.002 , adsurl =

2017 doi
[96]

ArXiv e-prints , archivePrefix = "arXiv", eprint =

Asteroid thermophysical modeling. ArXiv e-prints , archivePrefix = "arXiv", eprint =
[97]

Science , year = 2017, month = sep, volume = 357, pages =

Identification of a primordial asteroid family constrains the original planetesimal population. Science , year = 2017, month = sep, volume = 357, pages =. doi:10.1126/science.aam6036 , adsurl =

2017 doi
[98]

, archivePrefix = "arXiv", eprint =

Reconstructing the size distribution of the primordial Main Belt. , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2017.05.026 , adsurl =

2017 doi
[99]

The annual streams

Meteor stream activity I. The annual streams. , keywords =
[100]

, keywords =

NELIOTA: First temperature measurement of lunar impact flashes. , keywords =. doi:10.1051/0004-6361/201732109 , adsurl =

doi
[101]

, year = 2006, month = aug, volume = 183, pages =

Earth/Moon impact rate comparison: Searching constraints for lunar secondary/primary cratering proportion. , year = 2006, month = aug, volume = 183, pages =. doi:10.1016/j.icarus.2006.04.004 , adsurl =

2006 doi
[102]

NASA Special Publication , year = 1973, volume = 319, pages =

A Working List of Meteor Streams. NASA Special Publication , year = 1973, volume = 319, pages =

1973
[103]

, year = 2016, month = oct, volume = 538, pages =

Quantifying crater production and regolith overturn on the Moon with temporal imaging. , year = 2016, month = oct, volume = 538, pages =. doi:10.1038/nature19829 , adsurl =

2016 doi
[104]

, year = 2003, month = nov, volume = 426, pages =

The formation of the Kuiper belt by the outward transport of bodies during Neptune's migration. , year = 2003, month = nov, volume = 426, pages =

2003
[105]

Science , year = 2000, month = jun, volume = 288, pages =

Understanding the Distribution of Near-Earth Asteroids. Science , year = 2000, month = jun, volume = 288, pages =. doi:10.1126/science.288.5474.2190 , adsurl =

2000
[106]

Earth Moon and Planets , keywords =

Meteoroid Engineering Model (MEM): A Meteoroid Model For The Inner Solar System. Earth Moon and Planets , keywords =. doi:10.1007/s11038-005-9044-8 , adsurl =

doi
[107]

Icarus , year = 2002, month = apr, volume = 156, pages =

Debiased Orbital and Absolute Magnitude Distribution of the Near-Earth Objects. Icarus , year = 2002, month = apr, volume = 156, pages =. doi:10.1006/icar.2001.6788 , adsurl =

2002
[108]

Meteoritics and Planetary Science , year = 2000, month = nov, volume = 35, pages =

Source regions and time scales for the delivery of water to Earth. Meteoritics and Planetary Science , year = 2000, month = nov, volume = 35, pages =. doi:10.1111/j.1945-5100.2000.tb01518.x , adsurl =

2000
[109]

Nature Astronomy , year = 2017, month = mar, volume = 1, eid =

The pristine interior of comet 67P revealed by the combined Aswan outburst and cliff collapse. Nature Astronomy , year = 2017, month = mar, volume = 1, eid =. doi:10.1038/s41550-017-0092 , adsurl =

2017 doi
[110]

, year = 2016, month = feb, volume = 530, pages =

Super-catastrophic disruption of asteroids at small perihelion distances. , year = 2016, month = feb, volume = 530, pages =. doi:10.1038/nature16934 , adsurl =

2016 doi
[111]

, archivePrefix = "arXiv", eprint =

An anisotropic distribution of spin vectors in asteroid families. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201321993 , adsurl =

doi
[112]

Icarus , keywords =

A new investigation of hydration in the M-type asteroids. Icarus , keywords =. doi:10.1016/j.icarus.2015.01.021 , adsurl =

2015 doi
[113]

Meteoritics and Planetary Science , year = 1996, month = mar, volume =

Detailed data for 259 fireballs from the Canadian camera network and inferences concerning the influx of large meteoroids. Meteoritics and Planetary Science , year = 1996, month = mar, volume =. doi:10.1111/j.1945-5100.1996.tb02014.x , adsurl =

1996
[114]

, archivePrefix = "arXiv", eprint =

Lunar impact flashes from Geminids: analysis of luminous efficiencies and the flux of large meteoroids on Earth. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stv1921 , adsurl =

doi
[115]

, keywords =

A search for meteoritic flashes on the Moon. , keywords =
[116]

, year = 2000, month = jun, volume = 405, pages =

Optical detection of meteoroidal impacts on the Moon. , year = 2000, month = jun, volume = 405, pages =

2000
[117]

, keywords =

Observation and Interpretation of Leonid Impact Flashes on the Moon in 2001. , keywords =. doi:10.1086/341625 , adsurl =

2001 doi
[118]

Icarus , year = 2006, month = oct, volume = 184, pages =

Detection of sporadic impact flashes on the Moon: Implications for the luminous efficiency of hypervelocity impacts and derived terrestrial impact rates. Icarus , year = 2006, month = oct, volume = 184, pages =. doi:10.1016/j.icarus.2006.05.002 , adsurl =

2006 doi
[119]

Icarus , year = 2012, month = mar, volume = 218, pages =

Power and duration of impact flashes on the Moon: Implication for the cause of radiation. Icarus , year = 2012, month = mar, volume = 218, pages =. doi:10.1016/j.icarus.2011.11.028 , adsurl =

2012 doi
[120]

Icarus , archivePrefix = "arXiv", eprint =

The flux of kilogram-sized meteoroids from lunar impact monitoring. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2014.04.032 , adsurl =

2014 doi
[121]

, year = 2017, month = sep, volume = 143, pages =

A comparison of radiometric calibration techniques for lunar impact flashes. , year = 2017, month = sep, volume = 143, pages =. doi:10.1016/j.pss.2017.04.016 , adsurl =

2017 doi
[122]

, keywords =

Planetary Theories in rectangular and spherical variables: VSOP87 solution. , keywords =
[123]

, archivePrefix = "arXiv", eprint =

Analysis of Moon impact flashes detected during the 2012 and 2013 Perseids. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201525656 , adsurl =

2012 doi
[124]

Earth Moon and Planets , keywords =

First Lunar Flashes Observed from Morocco (ILIAD Network): Implications for Lunar Seismology. Earth Moon and Planets , keywords =. doi:10.1007/s11038-015-9462-1 , adsurl =

doi
[125]

, keywords =

MIDAS: Software for the detection and analysis of lunar impact flashes. , keywords =. doi:10.1016/j.pss.2015.03.018 , archivePrefix =. 1503.07018 , primaryClass =

2015 arXiv
[126]

, year = 2006, month = jun, volume =

The first confirmed Perseid lunar impact flash. , year = 2006, month = jun, volume =. doi:10.1016/j.icarus.2006.01.004 , adsurl =

2006 doi
[127]

, year = 2002, month = sep, volume =

Lightcurves of 1999 Leonid Impact Flashes on the Moon. , year = 2002, month = sep, volume =. doi:10.1006/icar.2002.6931 , adsurl =

1999
[128]

Earth Moon and Planets , keywords =

Ground-Based Observations Of Lunar Meteoritic Phenomena. Earth Moon and Planets , keywords =. doi:10.1023/B:MOON.0000047475.61749.c1 , adsurl =
[129]

Occultation Newsletter, International Occultation Timing Association (IOTA) , keywords =

Confirmed lunar meteor impacts from the November 1999 Leonids. Occultation Newsletter, International Occultation Timing Association (IOTA) , keywords =

1999
[130]

Meteoroids: The Smallest Solar System Bodies , year = 2011, editor =

Luminous Efficiency of Hypervelocity Meteoroid Impacts on the Moon Derived From the 2006 Geminids, 2007 Lyrids, and 2008 Taurids. Meteoroids: The Smallest Solar System Bodies , year = 2011, editor =

2006
[131]

, keywords =

The first observations to determine the temperature of a lunar impact flash and its evolution. , keywords =. doi:10.1093/mnras/sty1862 , archivePrefix =. 1807.03193 , primaryClass =

arXiv
[132]

, year = 1996, month = nov, volume = 78, pages =

Meteoroid Orbits. , year = 1996, month = nov, volume = 78, pages =. doi:10.1007/BF00171928 , adsurl =

1996 doi
[133]

Lunar and Planetary Science Conference , year = 2002, series =

Effect of Velocity and Angle on Light Intensity Generated by Hypervelocity Impacts. Lunar and Planetary Science Conference , year = 2002, series =

2002
[134]

36th Annual Lunar and Planetary Science Conference , year = 2005, series =

Investigations of the Luminous Energy and Luminous Efficiency of Experimental Impacts into Particulate Targets. 36th Annual Lunar and Planetary Science Conference , year = 2005, series =

2005
[135]

Lunar and Planetary Science Conference , year = 2004, series =

Early-Time Temperature Evolution of the Impact Flash and Beyond. Lunar and Planetary Science Conference , year = 2004, series =

2004
[136]

Earth Moon and Planets , keywords =

Observation and Interpretation of Meteoroid Impact Flashes on the Moon. Earth Moon and Planets , keywords =
[137]

, keywords =

Luminous Efficiency in Hypervelocity Impacts from the 1999 Lunar Leonids. , keywords =. doi:10.1086/312914 , adsurl =

1999 doi
[138]

, keywords =

Impact-induced thermal effects in the lunar and Mercurian regoliths. , keywords =. doi:10.1029/91JE02207 , adsurl =

doi
[139]

, year = 1961, month = apr, volume = 190, pages =

Comets and the Formation of Biochemical Compounds on the Primitive Earth. , year = 1961, month = apr, volume = 190, pages =. doi:10.1038/190389a0 , adsurl =

1961 doi
[140]

Science , keywords =

Mars and earth - Origin and abundance of volatiles. Science , keywords =. doi:10.1126/science.198.4316.453 , adsurl =

doi
[141]

Icarus , eprint =

Making other earths: dynamical simulations of terrestrial planet formation and water delivery. Icarus , eprint =. doi:10.1016/j.icarus.2003.11.019 , adsurl =

2003 doi
[142]

A radar survey of M- and X-class asteroids. III. Insights into their composition, hydration state, structure. Icarus , keywords =. doi:10.1016/j.icarus.2014.09.016 , adsurl =

2014 doi
[143]

Observations of Main-Belt Asteroids in the 3-MICRON Region
[144]

Planetary Space Science , year = 2011, month = jun, volume = 59, pages =

Mineralogical characterization of potential targets for the ASTEX mission scenario. Planetary Space Science , year = 2011, month = jun, volume = 59, pages =. doi:10.1016/j.pss.2011.03.005 , adsurl =

2011 doi
[145]

, year = 2015, month = dec, volume = 528, pages =

Sublimation in bright spots on (1) Ceres. , year = 2015, month = dec, volume = 528, pages =. doi:10.1038/nature15754 , adsurl =

2015 doi
[146]

Icarus , year = 2002, month = oct, volume = 159, pages =

Models of Twenty Asteroids from Photometric Data. Icarus , year = 2002, month = oct, volume = 159, pages =. doi:10.1006/icar.2002.6907 , adsurl =

2002
[147]

, keywords =

Motion of the asteroid (13206) 1997GC22 and the mass of (16) Psyche. , keywords =. doi:10.1051/0004-6361:20021444 , adsurl =

doi
[148]

Icarus , year = 1995, month = oct, volume = 117, pages =

Rotationally resolved spectra of asteroid 16 Psyche. Icarus , year = 1995, month = oct, volume = 117, pages =. doi:10.1006/icar.1995.1170 , adsurl =

1995
[149]

Icarus , year = 2005, month = may, volume = 175, pages =

Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroids. Icarus , year = 2005, month = may, volume = 175, pages =. doi:10.1016/j.icarus.2004.10.017 , adsurl =

2005 doi
[150]

Astronomical Journal , archivePrefix = "arXiv", eprint =

Detection of Rotational Spectral Variation on the M-type Asteroid (16) Psyche. Astronomical Journal , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-3881/153/1/29 , adsurl =

doi
[151]

Astronomical Journal , archivePrefix = "arXiv", eprint =

Detection of Water and/or Hydroxyl on Asteroid (16) Psyche. Astronomical Journal , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-3881/153/1/31 , adsurl =

doi
[152]

Summary and synthesis

A radar survey of M- and X-class asteroids II. Summary and synthesis. Icarus , year = 2010, month = jul, volume = 208, pages =. doi:10.1016/j.icarus.2010.01.017 , adsurl =

2010 doi
[153]

MNRS , keywords =

An analysis of the Hygiea asteroid family orbital region. MNRS , keywords =. doi:10.1093/mnras/stt437 , adsurl =

doi
[154]

, year = 2008, month = oct, volume = 197, pages =

On the origin of a double, oblique impact on Mars. , year = 2008, month = oct, volume = 197, pages =. doi:10.1016/j.icarus.2008.06.001 , adsurl =

2008 doi
[155]

, archivePrefix = "arXiv", eprint =

Discovery and Characteristics of the Rapidly Rotating Active Asteroid (62412) 2000 SY178 in the Main Belt. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-6256/149/2/44 , adsurl =

2000 doi
[156]

Icarus , keywords =

Asteroid (90) Antiope: Another icy member of the Themis family?. Icarus , keywords =. doi:10.1016/j.icarus.2015.03.008 , adsurl =

2015 doi
[157]

Lunar and Planetary Science Conference , year = 2016, series =

Asteroid (16) Psyche: The Science of Visiting a Metal World. Lunar and Planetary Science Conference , year = 2016, series =

2016
[158]

Icarus , keywords =

Radar observations and shape model of asteroid 16 Psyche. Icarus , keywords =. doi:10.1016/j.icarus.2016.08.011 , adsurl =

2016 doi
[159]

Icarus , archivePrefix = "arXiv", eprint =

Evidence of a metal-rich surface for the Asteroid (16) Psyche from interferometric observations in the thermal infrared. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2013.06.004 , adsurl =

2013 doi
[160]

, year = 2008, month = jul, volume = 72, pages =

Lunar rock-rain: Diverse silicate impact-vapor condensates in an Apollo-14 regolith breccia. , year = 2008, month = jul, volume = 72, pages =. doi:10.1016/j.gca.2008.04.031 , adsurl =

2008 doi
[161]

, keywords =

Mass and density of asteroids (16) Psyche and (121) Hermione. , keywords =
[162]

Astronomical Journal , keywords =

The Supplemental IRAS Minor Planet Survey. Astronomical Journal , keywords =. doi:10.1086/338320 , adsurl =

doi
[163]

Icarus , year = 2008, month = oct, volume = 197, pages =

Triaxial ellipsoid dimensions and rotational poles of seven asteroids from Lick Observatory adaptive optics images, and of Ceres. Icarus , year = 2008, month = oct, volume = 197, pages =. doi:10.1016/j.icarus.2008.05.009 , adsurl =

2008 doi
[164]

Icarus , archivePrefix = "arXiv", eprint =

Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2011.03.016 , adsurl =

2011 doi
[165]

Icarus , year = 2003, month = apr, volume = 162, pages =

Speckle interferometry observations of asteroids at tng*. Icarus , year = 2003, month = apr, volume = 162, pages =. doi:10.1016/S0019-1035(03)00006-X , adsurl =

2003 doi
[166]

Icarus , year = 2008, month = may, volume = 195, pages =

A radar survey of M- and X-class asteroids. Icarus , year = 2008, month = may, volume = 195, pages =. doi:10.1016/j.icarus.2007.11.032 , adsurl =

2008 doi
[167]

Icarus , archivePrefix = "arXiv", eprint =

Olivine-dominated asteroids: Mineralogy and origin. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2013.10.006 , adsurl =

2013 doi
[168]

Meteoritics and Planetary Science , year = 2001, month = mar, volume = 36, pages =

A new metal-rich chondrite grouplet. Meteoritics and Planetary Science , year = 2001, month = mar, volume = 36, pages =. doi:10.1111/j.1945-5100.2001.tb01882.x , adsurl =

2001
[169]

, year = 2006, month = feb, volume = 439, pages =

Iron meteorites as remnants of planetesimals formed in the terrestrial planet region. , year = 2006, month = feb, volume = 439, pages =. doi:10.1038/nature04536 , adsurl =

2006 doi
[170]

Icarus , keywords =

Surface properties of asteroids - A synthesis of polarimetry, radiometry, and spectrophotometry. Icarus , keywords =. doi:10.1016/0019-1035(75)90191-8 , adsurl =

doi
[171]

Icarus , keywords =

An extension of the Bus asteroid taxonomy into the near-infrared. Icarus , keywords =. doi:10.1016/j.icarus.2009.02.005 , adsurl =

2009 doi
[172]

Icarus , archivePrefix = "arXiv", eprint =

The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2013.06.027 , adsurl =

2013 doi
[173]

An analogue for low porosity targets

Survival of the impactor during hypervelocity collisions - I. An analogue for low porosity targets. MNRAS , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stv2844 , adsurl =

doi
[174]

An analogue for high-porosity targets

Survival of the impactor during hypervelocity collisions - II. An analogue for high-porosity targets. MNRAS , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stw2381 , adsurl =

doi
[175]

, keywords =

Very weak carbonaceous asteroid simulants I: Mechanical properties and response to hypervelocity impacts. , keywords =. doi:10.1016/j.icarus.2020.113648 , adsurl =

2020
[176]

Science , year = 2012, month = jun, volume = 336, pages =

Direct Detection of Projectile Relics from the End of the Lunar Basin-Forming Epoch. Science , year = 2012, month = jun, volume = 336, pages =. doi:10.1126/science.1219633 , adsurl =

2012 doi
[177]

Science , year = 2006, month = apr, volume = 312, pages =

A Population of Comets in the Main Asteroid Belt. Science , year = 2006, month = apr, volume = 312, pages =. doi:10.1126/science.1125150 , adsurl =

2006 doi
[178]

, year = 1950, month = jan, volume = 11, pages =

The structure of the cloud of comets surrounding the Solar System and a hypothesis concerning its origin. , year = 1950, month = jan, volume = 11, pages =

1950
[179]

Science , year = 2015, month = jan, volume = 347, number = 27, eid =

67P/Churyumov-Gerasimenko, a Jupiter family comet with a high D/H ratio. Science , year = 2015, month = jan, volume = 347, number = 27, eid =. doi:10.1126/science.1261952 , adsurl =

2015 doi
[180]

Astrophysical Journal , keywords =

The Lifetime of Ice on Main Belt Asteroids. Astrophysical Journal , keywords =. doi:10.1086/588633 , adsurl =

doi
[181]

, year = 2010, month = apr, volume = 464, pages =

Detection of ice and organics on an asteroidal surface. , year = 2010, month = apr, volume = 464, pages =. doi:10.1038/nature09028 , adsurl =

2010 doi
[182]

, year = 2010, month = apr, volume = 464, pages =

Water ice and organics on the surface of the asteroid 24 Themis. , year = 2010, month = apr, volume = 464, pages =. doi:10.1038/nature09029 , adsurl =

2010 doi
[183]

A & A , keywords =

(65) Cybele: detection of small silicate grains, water-ice, and organics. A & A , keywords =. doi:10.1051/0004-6361/201015339 , adsurl =

doi
[184]

, year = 2014, month = jan, volume = 505, pages =

Localized sources of water vapour on the dwarf planet (1)Ceres. , year = 2014, month = jan, volume = 505, pages =. doi:10.1038/nature12918 , adsurl =

2014 doi
[185]

ArXiv e-prints , archivePrefix = "arXiv", eprint =

Identification and Dynamical Properties of Asteroid Families. ArXiv e-prints , archivePrefix = "arXiv", eprint =
[186]

Icarus , year = 2007, month = mar, volume = 187, pages =

Nucleus properties of Comet 9P/Tempel 1 estimated from non-gravitational force modeling. Icarus , year = 2007, month = mar, volume = 187, pages =. doi:10.1016/j.icarus.2006.07.022 , adsurl =

2007 doi
[187]

The Astronomical Journal , eprint =

Light Curves of 20-100 km Kuiper Belt Objects Using the Hubble Space Telescope. The Astronomical Journal , eprint =. doi:10.1086/499228 , adsurl =

doi
[188]

MNRAS , year = 1853, month = apr, volume = 13, pages =

On the classification of comets and the distribution of their orbits in space. MNRAS , year = 1853, month = apr, volume = 13, pages =. doi:10.1093/mnras/13.6.188 , adsurl =

doi
[189]

A comet model. I. The acceleration of Comet Encke. The Astrophysical Journal , year = 1950, month = mar, volume = 111, pages =. doi:10.1086/145272 , adsurl =

1950 doi
[190]

A Comet Model. II. Physical Relations for Comets and Meteors. The Astrophysical Journal , year = 1951, month = may, volume = 113, pages =. doi:10.1086/145416 , adsurl =

1951 doi
[191]

The Astronomical Journal , keywords =

The Dynamical Structure of the Kuiper Belt. The Astronomical Journal , keywords =. doi:10.1086/117748 , adsurl =

doi
[192]

Icarus , year = 1997, month = may, volume = 127, pages =

From the Kuiper Belt to Jupiter-Family Comets: The Spatial Distribution of Ecliptic Comets. Icarus , year = 1997, month = may, volume = 127, pages =. doi:10.1006/icar.1996.5637 , adsurl =

1997
[193]

Icarus , year = 2002, month = aug, volume = 158, pages =

From Magnitudes to Diameters: The Albedo Distribution of Near Earth Objects and the Earth Collision Hazard. Icarus , year = 2002, month = aug, volume = 158, pages =. doi:10.1006/icar.2002.6887 , adsurl =

2002
[194]

The bulk statistics

Simulations of the population of Centaurs - I. The bulk statistics. MNRAS , eprint =. doi:10.1111/j.1365-2966.2004.08240.x , adsurl =

2004
[195]

Advances in Space Research , year = 1996, volume = 17, pages =

Use of combined light flash and plasma measurements to study hyper velocity impact processes. Advances in Space Research , year = 1996, volume = 17, pages =. doi:10.1016/0273-1177(95)00772-7 , adsurl =

1996 doi
[196]

, keywords =

A computer program for calculation of a theoretical meteor-stream radiant. , keywords =
[197]

Icarus , year = 1996, month = aug, volume = 122, pages =

Light Flash and Ionization from Hypervelocity Impacts on Ice. Icarus , year = 1996, month = aug, volume = 122, pages =. doi:10.1006/icar.1996.0129 , adsurl =

1996
[198]

Nature Geoscience , year = 2013, month = dec, volume = 6, pages =

Shock synthesis of amino acids from impacting cometary and icy planet surface analogues. Nature Geoscience , year = 2013, month = dec, volume = 6, pages =. doi:10.1038/ngeo1930 , adsurl =

2013 doi
[199]

Science , year = 1980, month = jun, volume = 208, pages =

Extraterrestrial Cause for the Cretaceous-Tertiary Extinction. Science , year = 1980, month = jun, volume = 208, pages =. doi:10.1126/science.208.4448.1095 , adsurl =

1980
[200]

, keywords =

Meteoroids detection with the LUMIO lunar CubeSat. , keywords =. doi:10.1016/j.icarus.2022.115213 , adsurl =

2022
[201]

Acta Astronautica , keywords =

LUMIO: A CubeSat for observing and characterizing micro-meteoroid impacts on the Lunar far side. Acta Astronautica , keywords =. doi:10.1016/j.actaastro.2022.03.032 , adsurl =

2022 doi
[202]

Acoustical Society of America Journal , year = 2001, month = may, volume =

Global infrasonic monitoring of large meteoroids. Acoustical Society of America Journal , year = 2001, month = may, volume =. doi:10.1121/1.4744344 , adsurl =

2001 doi
[203]

, keywords =

PyNAPLE: Lunar Surface Impact Crater Detection. , keywords =. doi:10.1093/mnras/stac1495 , archivePrefix =. 2204.12265 , primaryClass =

arXiv
[204]

, year = 2002, month = nov, volume =

The flux of small near-Earth objects colliding with the Earth. , year = 2002, month = nov, volume =. doi:10.1038/nature01238 , adsurl =

2002 doi
[205]

Journal of Geophysical Research (Planets) , keywords =

Moon meteoritic seismic hum: Steady state prediction. Journal of Geophysical Research (Planets) , keywords =. doi:10.1029/2008JE003294 , adsurl =

doi
[206]

, keywords =

Extending lunar impact flash observations into the daytime with short-wave infrared. , keywords =. doi:10.1093/mnras/stad2707 , archivePrefix =. 2308.00510 , primaryClass =

arXiv
[207]

, keywords =

Detection of small fresh craters on the Moon: Linking fresh craters to their lunar impact flash events. , keywords =. doi:10.1051/0004-6361/202555481 , adsurl =

doi
[208]

, keywords =

NELIOTA: New results and updated statistics after 6.5 years of lunar impact flashes monitoring. , keywords =. doi:10.1051/0004-6361/202449542 , archivePrefix =. 2403.19613 , primaryClass =

arXiv
[209]

, keywords =

Impacts on the Moon: Analysis methods and size distribution of impactors. , keywords =. doi:10.1016/j.pss.2021.105201 , archivePrefix =. 2111.15269 , primaryClass =

2021
[210]

, keywords =

SExtractor: Software for source extraction. , keywords =. doi:10.1051/aas:1996164 , adsurl =

doi
[211]

Icarus , keywords =

Velocity distributions among colliding asteroids. Icarus , keywords =. doi:10.1006/icar.1994.1021 , adsurl =

1994
[212]

GCA , year = 2006, month = dec, volume = 70, pages =

Extracting olivine (Fo Fa) compositions from Raman spectral peak positions. GCA , year = 2006, month = dec, volume = 70, pages =. doi:10.1016/j.gca.2006.07.035 , adsurl =

2006 doi
[213]

Icarus , archivePrefix = "arXiv", eprint =

The contamination of the surface of Vesta by impacts and the delivery of the dark material. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2014.02.021 , adsurl =

2014 doi
[214]

, archivePrefix = "arXiv", eprint =

Constraining the cometary flux through the asteroid belt during the late heavy bombardment. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201219296 , adsurl =

doi
[215]

Icarus , year = 2007, month = apr, volume = 187, pages =

Figure of the double Asteroid 90 Antiope from adaptive optics and lightcurve observations. Icarus , year = 2007, month = apr, volume = 187, pages =. doi:10.1016/j.icarus.2006.10.030 , adsurl =

2007 doi
[216]

Astronomical Journal , archivePrefix = "arXiv", eprint =

Rectified Asteroid Albedos and Diameters from IRAS and MSX Photometry Catalogs. Astronomical Journal , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-6256/140/4/933 , adsurl =

doi
[217]

, keywords =

Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey. , keywords =. doi:10.1093/pasj/63.5.1117 , adsurl =

doi
[218]

Icarus , archivePrefix = "arXiv", eprint =

Yarkovsky V-shape identification of asteroid families. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2016.09.029 , adsurl =

2016 doi
[219]

Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters. ApJ , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/741/2/68 , adsurl =

doi
[220]

, archivePrefix = "arXiv", eprint =

Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids. , archivePrefix = "arXiv", eprint =. doi:10.1088/2041-8205/759/1/L8 , adsurl =

doi
[221]

ApJ , archivePrefix = "arXiv", eprint =

Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos. ApJ , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/791/2/121 , adsurl =

doi
[222]

ApJ , archivePrefix = "arXiv", eprint =

NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos. ApJ , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/814/2/117 , adsurl =

doi
[223]

ArXiv e-prints , archivePrefix = "arXiv", eprint =

Volumes and bulk densities of forty asteroids from ADAM shape modeling. ArXiv e-prints , archivePrefix = "arXiv", eprint =
[224]

ArXiv e-prints , archivePrefix = "arXiv", eprint =

INPOP new release: INPOP13b. ArXiv e-prints , archivePrefix = "arXiv", eprint =
[225]

Icarus , archivePrefix = "arXiv", eprint =

Olivine on Vesta as exogenous contaminants brought by impacts: Constraints from modeling Vesta's collisional history and from impact simulations. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2016.07.009 , adsurl =

2016 doi
[226]

Icarus , year = 2011, month = jul, volume = 214, pages =

Cratering erosion of planetary embryos. Icarus , year = 2011, month = jul, volume = 214, pages =. doi:10.1016/j.icarus.2011.04.026 , adsurl =

2011 doi
[227]

Science , year = 1970, month = jun, volume = 168, pages =

Asteroid Vesta: Spectral Reflectivity and Compositional Implications. Science , year = 1970, month = jun, volume = 168, pages =. doi:10.1126/science.168.3938.1445 , adsurl =

1970
[228]

Science , year = 2012, month = may, volume = 336, pages =

Spectroscopic Characterization of Mineralogy and Its Diversity Across Vesta. Science , year = 2012, month = may, volume = 336, pages =. doi:10.1126/science.1219270 , adsurl =

2012 doi
[229]

P&SS , archivePrefix = "arXiv", eprint =

Density of asteroids. P&SS , archivePrefix = "arXiv", eprint =. doi:10.1016/j.pss.2012.03.009 , adsurl =

2012 doi
[230]

Science , year = 2012, month = may, volume = 336, pages =

Dawn at Vesta: Testing the Protoplanetary Paradigm. Science , year = 2012, month = may, volume = 336, pages =. doi:10.1126/science.1219381 , adsurl =

2012 doi
[231]

, year = 2012, month = nov, volume = 491, pages =

Dark material on Vesta from the infall of carbonaceous volatile-rich material. , year = 2012, month = nov, volume = 491, pages =. doi:10.1038/nature11561 , adsurl =

2012 doi
[232]

Science , year = 2012, month = may, volume = 336, pages =

Color and Albedo Heterogeneity of Vesta from Dawn. Science , year = 2012, month = may, volume = 336, pages =. doi:10.1126/science.1219088 , adsurl =

2012 doi
[233]

Icarus , year = 2014, month = sep, volume = 240, pages =

Composition and mineralogy of dark material units on Vesta. Icarus , year = 2014, month = sep, volume = 240, pages =. doi:10.1016/j.icarus.2014.04.040 , adsurl =

2014 doi
[234]

Icarus , archivePrefix = "arXiv", eprint =

Delivery of dark material to Vesta via carbonaceous chondritic impacts. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2012.08.011 , adsurl =

2012 doi
[235]

ArXiv e-prints , archivePrefix = "arXiv", eprint =

Spectral variability on primitive asteroids of the Themis and Beagle families: space weathering effects or parent body heterogeneity?. ArXiv e-prints , archivePrefix = "arXiv", eprint =
[236]

, keywords =

Hungaria asteroid region telescopic spectral survey (HARTSS) I: Stony asteroids abundant in the Hungaria background population. , keywords =. doi:10.1016/j.icarus.2016.11.002 , adsurl =

2016 doi
[237]

, year = 2008, month = jul, volume = 196, pages =

Visible and near infrared spectroscopic investigation of E-type asteroids, including 2867 Steins, a target of the Rosetta mission. , year = 2008, month = jul, volume = 196, pages =. doi:10.1016/j.icarus.2008.02.015 , adsurl =

2008 doi
[238]

ArXiv e-prints , archivePrefix = "arXiv", eprint =

Surface Albedo and Spectral Variability of Ceres. ArXiv e-prints , archivePrefix = "arXiv", eprint =
[239]

A changing amount of water ice?

Short-term variability on the surface of (1) Ceres . A changing amount of water ice?. A & A , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201425304 , adsurl =

doi
[240]

, year = 2011, month = oct, volume = 478, pages =

Ocean-like water in the Jupiter-family comet 103P/Hartley 2. , year = 2011, month = oct, volume = 478, pages =. doi:10.1038/nature10519 , adsurl =

2011 doi
[241]

Icarus , archivePrefix = "arXiv", eprint =

A new method to determine the grain size of planetary regolith. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2012.11.039 , adsurl =

2012 doi
[242]

Science , year = 2006, month = jun, volume = 312, pages =

Touchdown of the Hayabusa Spacecraft at the Muses Sea on Itokawa. Science , year = 2006, month = jun, volume = 312, pages =. doi:10.1126/science.1126164 , adsurl =

2006 doi
[243]

Science , year = 2001, month = apr, volume = 292, pages =

Imaging of Small-Scale Features on 433 Eros from NEAR: Evidence for a Complex Regolith. Science , year = 2001, month = apr, volume = 292, pages =. doi:10.1126/science.1058651 , adsurl =

2001 doi
[244]

, year = 2015, month = oct, volume = 526, pages =

Two independent and primitive envelopes of the bilobate nucleus of comet 67P. , year = 2015, month = oct, volume = 526, pages =. doi:10.1038/nature15511 , adsurl =

2015 doi
[245]

A & A , archivePrefix = "arXiv", eprint =

Comets as collisional fragments of a primordial planetesimal disk. A & A , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201526116 , adsurl =

doi
[246]

Icarus , archivePrefix = "arXiv", eprint =

Asteroid family ages. Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2015.04.041 , adsurl =

2015 doi
[247]

, archivePrefix = "arXiv", eprint =

Compositional characterisation of the Themis family. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201526962 , adsurl =

doi
[248]

Icarus , keywords =

The composition and origin of the C, P, and D asteroids - Water as a tracer of thermal evolution in the outer belt. Icarus , keywords =. doi:10.1016/0019-1035(90)90184-B , adsurl =

doi
[249]

GRL , keywords =

Geophysical evolution of the Themis family parent body. GRL , keywords =. doi:10.1029/2009GL042353 , adsurl =

doi
[250]

An infrared reflectance study of water in outer belt asteroids
[251]

, keywords =

A spectroscopic study of the THEMIS family. , keywords =. doi:10.1051/aas:1999150 , adsurl =

doi
[252]

Icarus , year = 2012, month = jun, volume = 219, pages =

Outer Main Belt asteroids: Identification and distribution of four 3- m spectral groups. Icarus , year = 2012, month = jun, volume = 219, pages =. doi:10.1016/j.icarus.2012.02.022 , adsurl =

2012 doi
[253]

Science , year = 2006, month = jun, volume = 312, pages =

The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa. Science , year = 2006, month = jun, volume = 312, pages =. doi:10.1126/science.1125841 , adsurl =

2006 doi
[255]

Astronomical Journal , archivePrefix = "arXiv", eprint =

Observational and Dynamical Characterization of Main-belt Comet P/2010 R2 (La Sagra). Astronomical Journal , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-6256/143/5/104 , adsurl =

2010 doi
[256]

Icarus , archivePrefix = "arXiv", eprint =

The nucleus of main-belt Comet P/2010 R2 (La Sagra). Icarus , archivePrefix = "arXiv", eprint =. doi:10.1016/j.icarus.2014.08.033 , adsurl =

2010 doi
[257]

, year = 2009, month = mar, volume = 458, pages =

The impact and recovery of asteroid 2008 TC _ 3. , year = 2009, month = mar, volume = 458, pages =. doi:10.1038/nature07920 , adsurl =

2008 doi
[258]

MAPS , year = 2010, month = oct, volume = 45, pages =

Asteroid 2008 TC _ 3 Almahata Sitta: A spectacular breccia containing many different ureilitic and chondritic lithologies. MAPS , year = 2010, month = oct, volume = 45, pages =. doi:10.1111/j.1945-5100.2010.01108.x , adsurl =

2008
[259]

Icarus , keywords =

A search for clustering among the meteoroid impacts detected by the Apollo lunar seismic network. Icarus , keywords =. doi:10.1016/0019-1035(91)90027-Q , adsurl =

doi
[260]

, year = 2013, month = dec, volume = 504, pages =

Olivine in an unexpected location on Vesta's surface. , year = 2013, month = dec, volume = 504, pages =. doi:10.1038/nature12665 , adsurl =

2013 doi
[261]

Meteoritics and Planetary Science , year = 2015, month = apr, volume = 50, pages =

Origin and history of ureilitic material in the solar system: The view from asteroid 2008 TC _ 3 and the Almahata Sitta meteorite. Meteoritics and Planetary Science , year = 2015, month = apr, volume = 50, pages =. doi:10.1111/maps.12401 , adsurl =

2008 doi
[262]

MNRAS , archivePrefix = "arXiv", eprint =

On the origin of the Almahata Sitta meteorite and 2008 TC _ 3 asteroid. MNRAS , archivePrefix = "arXiv", eprint =. doi:10.1111/j.1365-2966.2012.21220.x , adsurl =

2008
[263]

, keywords =

Measurements of the light flash produced by high velocity particle impact. , keywords =. doi:10.1016/0032-0633(75)90005-7 , adsurl =

doi
[264]

, keywords =

Analysis of the hypervelocity impact process from impact flash measurements. , keywords =. doi:10.1016/0032-0633(76)90114-8 , adsurl =

doi
[265]

, year = 1998, month = aug, volume = 46, pages =

Possible detection of meteor stream effects on the lunar sodium atmosphere. , year = 1998, month = aug, volume = 46, pages =. doi:10.1016/S0032-0633(98)00024-5 , adsurl =

1998 doi
[266]

, keywords =

Discovery of the distant lunar sodium tail and its enhancement following the Leonid Meteor Shower of 1998. , keywords =. doi:10.1029/1999GL900314 , adsurl =

1998 doi
[267]

Science , year = 2002, month = sep, volume = 297, pages =

Lead Isotopic Ages of Chondrules and Calcium-Aluminum-Rich Inclusions. Science , year = 2002, month = sep, volume = 297, pages =. doi:10.1126/science.1073950 , adsurl =

2002 doi
[268]

, keywords =

Densities and porosities of meteoroids. , keywords =. doi:10.1051/0004-6361:200810460 , adsurl =

doi
[269]

Asteroids III , year = 2002, pages =

Asteroid Space Weathering and Regolith Evolution. Asteroids III , year = 2002, pages =

2002
[270]

, year = 2009, month = apr, volume = 458, pages =

Solar wind as the origin of rapid reddening of asteroid surfaces. , year = 2009, month = apr, volume = 458, pages =. doi:10.1038/nature07956 , adsurl =

2009 doi
[271]

Icarus , year = 2009, month = aug, volume = 202, pages =

Plausible parent bodies for enstatite chondrites and mesosiderites: Implications for Lutetia's fly-by. Icarus , year = 2009, month = aug, volume = 202, pages =. doi:10.1016/j.icarus.2009.03.016 , adsurl =

2009 doi
[272]

Icarus , year = 2012, month = nov, volume = 221, pages =

High surface porosity as the origin of emissivity features in asteroid spectra. Icarus , year = 2012, month = nov, volume = 221, pages =. doi:10.1016/j.icarus.2012.04.003 , adsurl =

2012 doi
[273]

Meteoritics and Planetary Science , year = 2014, month = jan, volume = 49, pages =

Degree of impactor fragmentation under collision with a regolith surface Laboratory impact experiments of rock projectiles. Meteoritics and Planetary Science , year = 2014, month = jan, volume = 49, pages =. doi:10.1111/maps.12126 , adsurl =

2014 doi
[274]

Lunar and Planetary Science Conference , year = 2011, series =

Properties and Possible Origin of Black Boulders on the Asteroid Itokawa. Lunar and Planetary Science Conference , year = 2011, series =

2011
[275]

A & A , archivePrefix = "arXiv", eprint =

Puzzling asteroid 21 Lutetia: our knowledge prior to the Rosetta fly-by. A & A , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201013994 , adsurl =

doi
[276]

Planetary Space Science , year = 2012, month = jun, volume = 66, pages =

The geomorphology of (21) Lutetia: Results from the OSIRIS imaging system onboard ESA's Rosetta spacecraft. Planetary Space Science , year = 2012, month = jun, volume = 66, pages =. doi:10.1016/j.pss.2011.10.003 , adsurl =

2012 doi
[277]

Icarus , keywords =

Survivability of copper projectiles during hypervelocity impacts in porous ice: A laboratory investigation of the survivability of projectiles impacting comets or other bodies. Icarus , keywords =. doi:10.1016/j.icarus.2015.12.037 , adsurl =

2015 doi
[278]

Planetary Space Science , year = 2012, month = jun, volume = 66, pages =

Overview of Lutetia's surface composition. Planetary Space Science , year = 2012, month = jun, volume = 66, pages =. doi:10.1016/j.pss.2011.11.009 , adsurl =

2012 doi
[279]

Planetary Space Science , keywords =

Variegation and space weathering on asteroid 21 Lutetia. Planetary Space Science , keywords =. doi:10.1016/j.pss.2015.06.018 , adsurl =

2015 doi
[280]

Icarus , year = 1999, month = sep, volume = 141, pages =

On the Size Distribution of Asteroid Families: The Role of Geometry. Icarus , year = 1999, month = sep, volume = 141, pages =. doi:10.1006/icar.1999.6148 , adsurl =

1999
[281]

European Planetary Science Congress 2014 , year = 2014, month = apr, volume = 9, pages =

Characterisation of Raman spectra of high purity olivine as a function of temperature and shock history. European Planetary Science Congress 2014 , year = 2014, month = apr, volume = 9, pages =

2014
[282]

Bolides produced by impacts of large meteoroids into the Earth's atmosphere: comparison of theory with observations. I. Benesov bolide dynamics and fragmentation. A & A , keywords =
[283]

Science , year = 2000, month = may, volume = 288, pages =

Radar Observations of Asteroid 216 Kleopatra. Science , year = 2000, month = may, volume = 288, pages =. doi:10.1126/science.288.5467.836 , adsurl =

2000 doi
[284]

MNRAS , archivePrefix = "arXiv", eprint =

A large lunar impact blast on 2013 September 11. MNRAS , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stu083 , adsurl =

2013 doi
[285]

Icarus , keywords =

Mainbelt Asteroids: Results of Arecibo and Goldstone Radar Observations of 37 Objects during 1980-1995. Icarus , keywords =. doi:10.1006/icar.1999.6130 , adsurl =

1980
[286]

Science , keywords =

Mainbelt asteroids - Dual-polarization radar observations. Science , keywords =. doi:10.1126/science.229.4712.442 , adsurl =

doi
[287]

, pages=

Petrovic, J.J. , pages=. Journal of Materials Science , volume=. 2003 , issn=. doi:10.1023/A:1021134128038 , title=

2003 doi
[288]

, pages=

Petrovic, J.J. , pages=. Journal of Materials Science , volume=. 2001 , issn=. doi:10.1023/A:1017546429094 , title=

2001 doi
[289]

, title =

Schultz, Richard A. , title =. Journal of Geophysical Research: Planets , volume =. doi:10.1029/93JE00691 , pages =

doi
[290]

Measurement Science and Technology , year = 1999, month = jan, volume = 10, pages =

Hypervelocity impact studies using the 2 MV Van de Graaff accelerator and two-stage light gas gun of the University of Kent at Canterbury. Measurement Science and Technology , year = 1999, month = jan, volume = 10, pages =. doi:10.1088/0957-0233/10/1/011 , adsurl =

1999 doi
[291]

Asteroids III , year = 2002, pages =

Mineralogy of Asteroids. Asteroids III , year = 2002, pages =

2002
[292]

Hayhurst and Richard A

Colin J. Hayhurst and Richard A. Clegg. Cylindrically symmetric \ SPH\ simulations of hypervelocity impacts on thin plates. International Journal of Impact Engineering. 1997. doi:http://dx.doi.org/10.1016/S0734-743X(97)87505-7

1997 doi
[293]

Advances in Space Research , year = 2013, month = aug, volume = 52, pages =

Hydrocode modelling of hypervelocity impacts on ice. Advances in Space Research , year = 2013, month = aug, volume = 52, pages =. doi:10.1016/j.asr.2013.04.010 , adsurl =

2013 doi
[294]

Icarus , year = 2011, month = jul, volume = 214, pages =

Modeling the morphological diversity of impact craters on icy satellites. Icarus , year = 2011, month = jul, volume = 214, pages =. doi:10.1016/j.icarus.2011.04.015 , adsurl =

2011 doi
[295]

, pages=

Chopelas, A. , pages=. Physics and Chemistry of Minerals , volume=. 1990 , issn=. doi:10.1007/BF00199666 , title=

1990 doi
[296]

Journal of Mineralogical and Petrological Sciences , volume=

Raman spectroscopic study of olivine-group minerals , author=. Journal of Mineralogical and Petrological Sciences , volume=. 2008 , publisher=

2008
[297]

Foster and P.J

N.F. Foster and P.J. Wozniakiewicz and M.C. Price and A.T. Kearsley and M.J. Burchell. Identification by Raman spectroscopy of Mg–Fe content of olivine samples after impact at 6 km s−1 onto aluminium foil and aerogel: In the laboratory and in Wild-2 cometary samples....

2013 doi
[298]

Meteoritics and Planetary Science , keywords =

In situ analysis of residues resulting from laboratory impacts into aluminum 1100 foil: Implications for Stardust crater analyses. Meteoritics and Planetary Science , keywords =. doi:10.1111/j.1945-5100.2009.tb01191.x , adsurl =

1945
[299]

, archivePrefix = "arXiv", eprint =

Comet-like mineralogy of olivine crystals in an extrasolar proto-Kuiper belt. , archivePrefix = "arXiv", eprint =. doi:10.1038/nature11469 , adsurl =

doi
[300]

Science , year = 2006, month = dec, volume = 314, pages =

Mineralogy and Petrology of Comet 81P/Wild 2 Nucleus Samples. Science , year = 2006, month = dec, volume = 314, pages =. doi:10.1126/science.1135842 , adsurl =

2006 doi

Pith tools

Reviewed August 3, 2026 · model on record in the stance chip above.

[1] [1]

JPL , year = 2016, url =

2016

[2] [2]

AIDA Study , year = 2016, url =

2016

[3] [3]

DAWN mission , year = 2016, url =

2016

[4] [4]

Asteroid Physical Properties, ESA , year = 2017, url =

2017

[5] [5]

Ruff Database , year = 2016, url =

2016

[6] [6]

Asteroids III, W

Meteoritic Parent Bodies: Their Number and Identification. Asteroids III, W. F. Bottke Jr., A. Cellino, P. Paolicchi, and R. P. Binzel (eds), University of Arizona Press, Tucson, p.653-667 , year = 2002, editor =

2002

[7] [7]

Asteroids IV , year = 2015, editor =

Astronomical Observations of Volatiles on Asteroids. Asteroids IV , year = 2015, editor =. doi:10.2458/azu_uapress_9780816532131-ch004 , adsurl =

work page doi:10.2458/azu_uapress_9780816532131-ch004 2015

[8] [8]

doi:10.1007/978-1-4419-0324-2 , adsurl =

Lunar Meteoroid Impacts and How to Observe Them. doi:10.1007/978-1-4419-0324-2 , adsurl =

work page doi:10.1007/978-1-4419-0324-2