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REVIEW 2 major objections 4 minor 48 references

A Space Mission to Earth's Nearest Black Hole: Reality or Science Fiction?

T0 review · 2 major / 4 minor · reviewed 2026-07-14 · grok-4.5

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Pith's one-line read A laser-propelled nanocraft mission to the nearest black hole could test Kerr spacetime at 10^{-6} precision within a century.

desk verdict A clear, carefully hedged conference talk that packages known population estimates and laser-sail ideas into a black-hole mission roadmap; useful as advocacy, not as a new result. read the letter →

arxiv 2607.10982 v1 pith:XMHFK7EC submitted 2026-07-13 gr-qc astro-ph.HE

Cosimo Bambi This is my paper
classification gr-qcastro-ph.HE PACS 04.70.-s04.80.Cc95.55.Pe97.60.Lf
keywords interstellarmissionnanocraftlaserpropulsionisolatedblackholesKerrmetrictestsflybyexperimentslocalmediumstrong-fieldgravity
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

Remote observations of black holes will never match the precision of atomic or particle physics, because their environments are complex and beyond our control. This talk argues that an in-situ interstellar mission is not pure science fiction: stellar-mass black holes may lie as close as ~7 pc, laser-driven gram-scale nanocrafts could reach one-third light speed, and a 20–25 light-year trip would take 60–75 years of coasting followed by 20–25 years for data return, for a total mission of 80–100 years. Flyby probes that pass near the critical radii separating capture from escape could measure deviations from the Kerr metric beyond the first post-Newtonian order at the 10^{-6} level—orders of magnitude tighter than present or planned remote constraints. Intermediate steps such as discovering an isolated black hole accreting from the local interstellar medium and developing the nanocraft technology itself already have independent scientific value.

What carries the argument

Laser-propelled nanocraft (gram-scale wafer plus meter-scale lightsail) performing flybys near the critical impact parameters that separate trajectories returning to infinity from those captured by the black hole.

What would settle it

A multi-wavelength campaign of the shortlist of high-proper-motion IR/optical sources inside the Local Interstellar Clouds that either identifies a nearby isolated accreting black hole or rules out all candidates within 15 pc, combined with demonstration that nanocrafts cannot be guided or released close enough to critical impact parameters.

Watch

Extended reading notes

Core claim

An interstellar mission with laser-propelled nanocrafts to a black hole at 20–25 light-years, traveling at roughly one-third the speed of light, is technologically plausible within a few decades and could deliver in-situ tests of the Kerr metric and the existence of an event horizon at precision unattainable by remote astronomy.

Load-bearing premise

A stellar-mass black hole must exist within roughly 20–25 light-years and be located and tracked with enough accuracy for a nanocraft or its sub-probes to pass sufficiently close to the critical radii.

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Editorial analysis

A structured set of objections, weighed in public.

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

Referee Report

2 major / 4 minor

Summary. This conference contribution (Mondello Workshop 2026) argues that an interstellar mission with laser-propelled nanocrafts to a stellar-mass black hole at 20–25 light-years is not impossible. Using population estimates from Olejak et al. (2020) and a simple Galactic-disk volume model, it places the nearest black hole within ~7 pc and ~10 objects within 15 pc. It outlines a multi-wavelength search strategy for isolated black holes accreting from Local Interstellar Clouds, sketches a laser-sail nanocraft architecture capable of ~c/3, and estimates an 80–100 year mission timeline. Citing companion calculations, it claims that flyby experiments near critical impact parameters with cm-scale probes could constrain Kerr deviations beyond the first post-Newtonian order at the 10^{-6} level—orders of magnitude better than current or near-future remote observations. The text is carefully hedged as speculative advocacy rather than a detailed mission design.

Significance. If the population estimate holds and a nearby isolated black hole can be identified, the paper correctly identifies a unique scientific opportunity: in-situ strong-field tests of the Kerr metric and event-horizon existence that remote observations are unlikely to match in precision. The synthesis of existing population models, accretion-search strategies, and laser-sail concepts into a concrete multi-decade roadmap is useful for the community. Explicit credit is due for the transparent order-of-magnitude volume argument, the clear separation of free parameters (speed, acceleration, Galactic BH number), and the honest acknowledgment that deceleration remains unsolved while still showing that pure flybys can suffice. The intermediate milestones (discovery of an accreting isolated BH, Solar-System-boundary probes) are independently valuable.

major comments (2)
  1. Sections 2 and 4: the central feasibility claim rests on the existence of a black hole at 20–25 ly with usable astrometry. The 7 pc / 15 pc figures are correctly labeled order-of-magnitude (cylinder volume ~150 kpc^{3} divided by 10^{8} objects), yet the mission timeline and flyby geometry assume a concrete target at that distance. The manuscript should quantify how the scientific return degrades if the nearest object is instead at 40–50 ly, or state explicitly that the 80–100 yr figure is conditional on a discovery within ~25 ly.
  2. Section 5 and the Gokus discussion reply: the 10^{-6} accuracy claim for flybys is taken from the companion note [48] and is load-bearing for the scientific justification. That note assumes probes can be placed near the critical impact parameters that separate capture from scattering trajectories. The present text does not demonstrate (or even sketch) a terminal-guidance or sub-probe-release architecture that achieves the required impact-parameter precision without deceleration. A short quantitative statement of the required delivery accuracy (or an explicit caveat that this remains an open engineering problem) is needed before the precision claim can be used as a primary motivation.
minor comments (4)
  1. Figure 1 caption and surrounding text: the Local Interstellar Clouds are modeled as 3 pc spheres; a one-sentence note on how sensitive the detection prospects are to this geometric idealization would help.
  2. Section 3: the multi-wavelength selection pipeline (CatWISE2020 + NSC DR2) is described at a high level; a brief pointer to the expected false-positive rate or to the forthcoming Nosirov et al. paper would strengthen the claim that candidates can be isolated.
  3. Throughout: several companion arXiv notes ([18], [19], [47], [48], [35]) are cited as the technical backbone; ensuring that the key numerical claims (10^{-6}, critical radii) are self-contained or at least summarized with their main assumptions would improve readability for a conference audience.
  4. Typographical: occasional missing spaces after periods and in compound adjectives (e.g., “blackhole” vs “black hole”) appear in the compiled text; a light copy-edit pass is recommended.

Circularity Check

1 steps flagged · score 2.0 of 10

No significant circularity: speculative roadmap with self-citations to independent companion calculations, not tautological redefinitions.

  1. self citation load bearing [Section 5 (Experiments Near the Black Hole), paragraphs on flyby accuracy]
    "The study in Ref. [48] considers the opposite situation: we cannot decelerate the nanocrafts and must instead perform flyby experiments. It turns out that very precise and accurate flyby experiments are possible if we have the capability of sending some probes near the critical radii that separate trajectories returning to infinity from those that fall onto the black hole. The conclusion of Ref. [48] is that tiny probes with a size of ∼1 cm may potentially test deviations from the predictions of General Relativity beyond the first post-Newtonian order with an accuracy at the level of 10^{-6}."

    The paper’s strongest quantitative scientific-return claim (10^{-6} accuracy on Kerr deviations) rests entirely on the author’s own concurrent arXiv note [48] rather than an external derivation or independent calculation reproduced here. This is self-citation that is load-bearing for the precision figure, but the cited work is an independent calculation of flyby trajectories, not a redefinition or fitted tautology of the present text; hence only minor circularity.

full rationale

This is a conference talk synthesizing external population estimates (Olejak et al. 2020), ISM accretion literature, and laser-sail concepts into a hedged feasibility argument. The central claims (BH density ~1 per 1500 pc^{3} implying possible objects within ~7–15 pc; 80–100 yr mission at ~1/3 c; flyby tests at ~10^{-6} accuracy) are order-of-magnitude estimates or results imported from companion notes [47,48] by the same author. Those notes are presented as independent preliminary calculations of orbiting/flyby experiments, not as uniqueness theorems or fitted parameters that force the present conclusions by construction. No equation in the text equates a claimed prediction to a fitted free parameter or to a definitional identity. Self-citation is present and load-bearing for the precision claim, but does not reduce the argument to a tautology; the paper remains self-contained as advocacy of a speculative program. Score 2 reflects only the minor self-citation pattern, consistent with an honest non-finding of circularity.

Assumptions & free parameters 3 free parameters · 4 assumptions · 0 invented entities

The central feasibility claim rests on standard astrophysical population models, the existence of laser-sail technology extrapolated from Starshot-class concepts, and idealized probe trajectories near a Kerr black hole. No new free parameters are fitted to data in this text; numbers are taken from literature or chosen as illustrative targets (1/3 c, 20–25 ly). No new physical entities are postulated.

free parameters (3)
  • target nanocraft speed = c/3
    Chosen as one-third the speed of light for the 80–100 year timeline; higher speeds raise cost but are not derived.
  • maximum acceleration = 1e5 m/s^2
    Assumed a_max ≈ 10^5 m s^{-2} to set the ~17-minute boost phase; engineering target, not measured.
  • Galactic-disk black-hole number = 1.0e8
    Taken from Olejak et al. 2020 (1.0e8 in the disk); used to compute local density.
assumptions (4)
  • domain assumption Stellar-mass black holes form from stars ≳20 M_⊙ and number ~10^8–10^9 in the Galaxy, mostly isolated.
    Section 2; taken from Timmes et al. and Olejak et al. without re-derivation.
  • domain assumption Laser radiation pressure on a dielectric lightsail can accelerate a gram-scale craft to a significant fraction of c without carrying propellant.
    Section 4; standard lightsail physics (Marx, Lubin, Starshot).
  • domain assumption In 4D GR without exotic matter the end-state of collapse is a Kerr black hole characterized only by mass and spin.
    Section 5; standard uniqueness theorems.
  • ad hoc to paper Flyby trajectories near the critical impact parameter can constrain post-Newtonian deviations at the 10^{-6} level with cm-scale probes.
    Section 5 and Ref. [48]; preliminary calculation not independently verified in this text.

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Cite this review

Pith. "Pith review of A Space Mission to Earth's Nearest Black Hole: Reality or Science Fiction?." pith.science (2026). https://pith.science/paper/XMHFK7EC

@misc{pith2026260710982,
  author       = {Pith},
  title        = {Pith review of: A Space Mission to Earth's Nearest Black Hole: Reality or Science Fiction?},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/XMHFK7EC}},
  note         = {Machine review of arXiv:2607.10982}
}
read the original abstract

Black holes are the sources of the strongest gravitational fields in the present-day Universe, offering unparalleled opportunities to test Einstein's theory of General Relativity in the strong-field regime. In this talk, I will examine the prospect of sending small spacecraft on an interstellar mission to the nearest black hole. While highly speculative and fraught with technical challenges, such an endeavor is not entirely beyond the realm of possibility. Although the necessary technology does not yet exist, it may become available within the next 20 to 30 years. The mission itself could span 80 to 100 years, yet the scientific return would be profound and potentially unattainable through other means.

Figures

Figures reproduced from arXiv: 2607.10982 by the authors.

Figure 1
Figure 1. Three-dimensional map of the local region within 15 pc of the Solar System. The Sun is at the center and is indicated by the black star. The Local Interstellar Clouds are modeled as spheres of radius 3 pc, and the legend reports their abbreviated names. Figure courtesy of Abdurakhmon Nosirov. In Ref. [35], we propose a method to find candidate isolated black holes in nearby clouds. We start from the all-sky IR catal… view at source ↗
Figure 2
Figure 2. Sketch of a nanocraft. Figure from Ref. [18]. 4. Interstellar Mission The closest star to the Solar System is Proxima Centauri, which lies 4.24 light-years from the Sun. It is thus clear that exploration beyond the Solar System requires the development of spacecraft that can travel at some significant fraction of the speed of light. Current chemically propelled spacecraft cannot achieve this, as can be readily seen … view at source ↗
Figure 3
Figure 3. Phases of a hypothetical interstellar mission with a nanocraft to the closest black hole. Figure from Ref. [18]. nanocraft to its target speed. There are no fundamental barriers preventing the attainment of 90% of the speed of light using this approach, although higher velocities immediately increase mission costs. Since the nanocraft does not carry any fuel (the lasers are located on the ground or in space), it is … view at source ↗

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Works this paper leans on

48 extracted references · 7 canonical work pages

  1. [48]

    Testing Black Holes with Interstellar Missions: II. Flyby Probes

    Y.Fan,C.Bambi,L.Gao,A.NosirovandA.Santangelo,TestingBlackHoleswithInterstellar Missions: II. Flyby Probes, https://doi.org/10.48550/arXiv.2607.09077 [arXiv:2607.09077 [gr-qc]]. DISCUSSION ANDREA GOKUS:How much do the orbital motions of a black hole with respect to the Solar System need to be taken into account? Will it be possible to achieve the accuracy ...

    work page Pith review arXiv doi:10.48550/arxiv.2607.09077

  2. [1]

    C. E. Rhoades, Jr. and R. Ruffini,Maximum mass of a neutron star, Phys. Rev. Lett.32, 324-327 (1974) https://doi.org/10.1103/PhysRevLett.32.324

    doi:10.1103/physrevlett.32.324 1974

  3. [2]

    62, 485-515 (2012) https://doi.org/10.1146/annurev-nucl-102711-095018 [arXiv:1305.3510 [nucl-th]]

    J.M.Lattimer,Thenuclearequationofstateandneutronstarmasses,Ann.Rev.Nucl.Part.Sci. 62, 485-515 (2012) https://doi.org/10.1146/annurev-nucl-102711-095018 [arXiv:1305.3510 [nucl-th]]

    arXiv doi:10.1146/annurev-nucl-102711-095018 2012

  4. [3]

    Maoz,Dynamical constraints on alternatives to massive black holes in galactic nu- clei, Astrophys

    E. Maoz,Dynamical constraints on alternatives to massive black holes in galactic nu- clei, Astrophys. J. Lett.494, L181-L184 (1998) https://doi.org/10.1086/311194 [arXiv:astro- ph/9710309 [astro-ph]]

    doi:10.1086/311194 1998

  5. [4]

    Bambi,Testing black hole candidates with electromagnetic radiation, Rev

    C. Bambi,Testing black hole candidates with electromagnetic radiation, Rev. Mod. Phys.89, 025001 (2017), https://doi.org/10.1103/RevModPhys.89.025001 [arXiv:1509.03884 [gr-qc]]

    arXiv doi:10.1103/revmodphys.89.025001 2017

  6. [5]

    C. Bambi,Black Holes: A Laboratory for Testing Strong Gravity(Springer Sin- gapore, 2017), ISBN 978-981-10-4523-3, 978-981-13-5158-7, 978-981-10-4524-0, https://doi.org/10.1007/978-981-10-4524-0

    doi:10.1007/978-981-10-4524-0 2017

  7. [6]

    B. P. Abbottet al.[LIGO Scientific and Virgo],Tests of general relativity with GW150914, Phys. Rev. Lett.116, 221101 (2016) [erratum: Phys. Rev. Lett.121, 129902 (2018)] https://doi.org/10.1103/PhysRevLett.116.221101 [arXiv:1602.03841 [gr-qc]]

    arXiv doi:10.1103/physrevlett.116.221101 2016

  8. [7]

    Yunes, K

    N. Yunes, K. Yagi and F. Pretorius,Theoretical Physics Implications of the Binary Black-Hole Mergers GW150914 and GW151226, Phys. Rev. D94, 084002 (2016) https://doi.org/10.1103/PhysRevD.94.084002 [arXiv:1603.08955 [gr-qc]]. 8 A Space Mission to Earth’s Nearest Black HoleCosimo Bambi

    arXiv doi:10.1103/physrevd.94.084002 2016

Show all 48 references
  1. [8]

    B. P. Abbottet al.[LIGO Scientific and Virgo],Tests of General Relativity with the Binary BlackHoleSignalsfromtheLIGO-VirgoCatalogGWTC-1,Phys.Rev.D100,104036(2019) https://doi.org/10.1103/PhysRevD.100.104036 [arXiv:1903.04467 [gr-qc]]

    2019 doi arXiv

  2. [9]

    D.Das,S.ShashankandC.Bambi,ImprovedConstraintsonNon-KerrDeviationsfromBinary Black Hole Inspirals Using GWTC-4 Data, EPJC (in press) [arXiv:2604.15965 [gr-qc]]

    arXiv

  3. [10]

    Z. Cao, S. Nampalliwar, C. Bambi, T. Dauser and J. A. Garcia,Testing general relativity with the reflection spectrum of the supermassive black hole in 1H0707−495, Phys. Rev. Lett.120, 051101 (2018) https://doi.org/10.1103/PhysRevLett.120.051101 [arXiv:1709.00219 [gr-qc]]

    2018 doi arXiv

  4. [11]

    A.Tripathi,S.Nampalliwar,A.B.Abdikamalov,D.Ayzenberg,C.Bambi,T.Dauser,J.A.Gar- ciaandA.Marinucci,TowardPrecisionTestsofGeneralRelativitywithBlackHoleX-RayRe- flectionSpectroscopy,Astrophys.J.875,56(2019)https://doi.org/10.3847/1538-4357/ab0e7e [arXiv:1811.08148 [gr-qc]]

    2019 doi arXiv

  5. [12]

    Tripathi, A

    A. Tripathi, A. B. Abdikamalov, D. Ayzenberg, C. Bambi, V. Grinberg and M. Zhou,Testing the Kerr Black Hole Hypothesis with GX 339–4 by a Combined Analysis of Its Thermal SpectrumandReflectionFeatures,Astrophys.J.907,31(2021)https://doi.org/10.3847/1538- 4357/abccbd [arXiv:201...

    2021 doi arXiv

  6. [13]

    Tripathi, Y

    A. Tripathi, Y. Zhang, A. B. Abdikamalov, D. Ayzenberg, C. Bambi, J. Jiang, H. Liu and M.Zhou,TestingGeneralRelativitywithNuSTARdataofGalacticBlackHoles,Astrophys.J. 913, 79 (2021) https://doi.org/10.3847/1538-4357/abf6cd [arXiv:2012.10669 [astro-ph.HE]]

    2021 doi arXiv

  7. [14]

    Bambi,Testing Gravity with Black Hole X-Ray Data, inRecent Progress on Gravity Tests: Challenges and Future Perspectives(Eds

    C. Bambi,Testing Gravity with Black Hole X-Ray Data, inRecent Progress on Gravity Tests: Challenges and Future Perspectives(Eds. C. Bambi and A. Cardenas-Avendano, Springer Singapore, 2024) https://doi.org/10.1007/978-981-97-2871-8_5 [arXiv:2210.05322 [gr-qc]]

    2024 doi arXiv

  8. [15]

    Psaltiset al.[Event Horizon Telescope],Gravitational Test Beyond the First Post- Newtonian Order with the Shadow of the M87 Black Hole, Phys

    D. Psaltiset al.[Event Horizon Telescope],Gravitational Test Beyond the First Post- Newtonian Order with the Shadow of the M87 Black Hole, Phys. Rev. Lett.125, 141104 (2020) https://doi.org/10.1103/PhysRevLett.125.141104 [arXiv:2010.01055 [gr-qc]]

    2020 doi arXiv

  9. [16]

    Akiyamaet al.[Event Horizon Telescope],First Sagittarius A* Event Horizon Tele- scope Results

    K. Akiyamaet al.[Event Horizon Telescope],First Sagittarius A* Event Horizon Tele- scope Results. VI. Testing the Black Hole Metric, Astrophys. J. Lett.930, L17 (2022) https://doi.org/10.3847/2041-8213/ac6756 [arXiv:2311.09484 [astro-ph.HE]]

    2022 doi arXiv

  10. [17]

    Vagnozzi, R

    S. Vagnozzi, R. Roy, Y. D. Tsai, L. Visinelli, M. Afrin, A. Allahyari, P. Bambhaniya, D. Dey, S. G. Ghosh and P. S. Joshi,et al. Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A∗, Class. Quant. Grav.40, 165...

    2023 doi arXiv

  11. [18]

    C.Bambi,Aninterstellarmissiontotestastrophysicalblackholes,iScience28,113142(2025), https://doi.org/10.1016/j.isci.2025.113142 [arXiv:2504.14576 [gr-qc]]

    2025 doi

  12. [19]

    Bambi,An interstellar mission to the closest black hole?, https://doi.org/10.48550/arXiv.2509.11222 [arXiv:2509.11222 [gr-qc]]

    C. Bambi,An interstellar mission to the closest black hole?, https://doi.org/10.48550/arXiv.2509.11222 [arXiv:2509.11222 [gr-qc]]. 9 A Space Mission to Earth’s Nearest Black HoleCosimo Bambi

    doi arXiv

  13. [20]

    Bambi,Stellar-Mass Black Holes, Symmetry17, 1393 (2025), https://doi.org/10.3390/sym17091393 [arXiv:2507.15270 [astro-ph.HE]]

    C. Bambi,Stellar-Mass Black Holes, Symmetry17, 1393 (2025), https://doi.org/10.3390/sym17091393 [arXiv:2507.15270 [astro-ph.HE]]

    2025 doi arXiv

  14. [21]

    F. X. Timmes, S. E. Woosley and T. A. Weaver,The Neutron star and black hole initial mass function, Astrophys. J.457, 834 (1996), https://doi.org/10.1086/176778 [arXiv:astro- ph/9510136 [astro-ph]]

    1996 doi

  15. [22]

    Olejak, K

    A. Olejak, K. Belczynski, T. Bulik and M. Sobolewska,Synthetic catalog of black holes in the Milky Way, Astron. Astrophys.638, A94 (2020), https://doi.org/10.1051/0004- 6361/201936557 [arXiv:1908.08775 [astro-ph.SR]]

    2020 doi arXiv

  16. [23]

    430, 1538 (2013), https://doi.org/10.1093/mnras/sts688 [arXiv:1301.1341 [astro-ph.HE]]

    R.Fender,T.MaccaroneandI.Heywood,Theclosestblackholes,Mon.Not.Roy.Astron.Soc. 430, 1538 (2013), https://doi.org/10.1093/mnras/sts688 [arXiv:1301.1341 [astro-ph.HE]]

    2013 doi arXiv

  17. [24]

    J.Lett.988,L12(2025),https://doi.org/10.3847/2041-8213/ade7f8[arXiv:2506.20711[astro- ph.GA]]

    L.MurchikovaandK.C.Sahu,ObservabilityofIsolatedStellar-massBlackHoles,Astrophys. J.Lett.988,L12(2025),https://doi.org/10.3847/2041-8213/ade7f8[arXiv:2506.20711[astro- ph.GA]]

    2025 doi arXiv

  18. [25]

    Nosirov, C

    A. Nosirov, C. Bambi, L. Gao, J. de Bruijne, J. Jiang, A. Santangelo and F. G. Xie,Search- ing for Isolated Black Hole Candidates within 15 pc of the Solar System in Gaia DR3, Astrophys. J.1004, 21 (2026), https://doi.org/10.3847/1538-4357/ae6805 [arXiv:2601.14499 [astro-ph.HE]]

    2026 doi arXiv

  19. [26]

    V. F. Shvartsman, Soviet Astron. AJ15, 377 (1971)

    1971

  20. [27]

    Meszaros,Radiation from spherical accretion onto black holes, Astron

    P. Meszaros,Radiation from spherical accretion onto black holes, Astron. Astrophys.44, 59-68 (1975)

    1975

  21. [28]

    McDowell,Accretion radiation from nearby isolated black holes, Mon

    J. McDowell,Accretion radiation from nearby isolated black holes, Mon. Not. Roy. Astron. Soc.217, 77-85 (1985) https://doi.org/10.1093/mnras/217.1.77

    1985 doi

  22. [29]

    Fujita, S

    Y. Fujita, S. Inoue, T. Nakamura, T. Manmoto and K. E. Nakamura,Emission from isolated blackholesandMACHOsaccretingfromtheinterstellarmedium,Astrophys.J.Lett.495,L85 (1998) https://doi.org/10.1086/311220 [arXiv:astro-ph/9712284 [astro-ph]]

    1998 doi arXiv

  23. [30]

    T. J. Maccarone,Using radio emission to detect isolated and quiescent accreting black holes, Mon.Not.Roy.Astron.Soc.360,30(2005)https://doi.org/10.1111/j.1745-3933.2005.00039.x [arXiv:astro-ph/0503097 [astro-ph]]

    2005 doi

  24. [31]

    Tsuna, N

    D. Tsuna, N. Kawanaka and T. Totani,X-ray Detectability of Accreting Isolated Black Holes in Our Galaxy, Mon. Not. Roy. Astron. Soc.477, 791-801 (2018) https://doi.org/10.1093/mnras/sty699 [arXiv:1801.04667 [astro-ph.HE]]

    2018 doi arXiv

  25. [32]

    10 A Space Mission to Earth’s Nearest Black HoleCosimo Bambi

    F.Scarcella,D.Gaggero,R.Connors,J.Manshanden,M.RicottiandG.Bertone,Multiwave- lengthdetectabilityofisolatedblackholesintheMilkyWay,Mon.Not.Roy.Astron.Soc.505, 4036-4047(2021)https://doi.org/10.1093/mnras/stab1533[arXiv:2012.10421[astro-ph.HE]]. 10 A Space Mission to Earth’s Ne...

    2021 doi arXiv

  26. [33]

    J. R. Martinez, V. Bosch-Ramon, F. L. Vieyro and S. del Palacio,Probing the detectability of electromagnetic signatures from Galactic isolated black holes, Astron. Astrophys.700, A49 (2025) https://doi.org/10.1051/0004-6361/202554910 [arXiv:2506.23427 [astro-ph.HE]]

    2025 doi arXiv

  27. [34]

    Redfield and R

    S. Redfield and R. E. Falcon,The Structure of the Local Interstellar Medium V: Electron Densities, Astrophys. J.673, 283 (2008) https://doi.org/10.1086/524002 [arXiv:0804.1802 [astro-ph]]

    2008 doi arXiv

  28. [35]

    Nosirov, C

    A. Nosirov, C. Bambi,et al., (in preparation)

  29. [36]

    G.Dyson,ProjectOrion: TheTrueStoryoftheAtomicSpaceship(HenryHoltandCo,2002), ISBN 978-0805059854

    2002

  30. [37]

    K. F. Long and P. R. Galea,Project Daedalus: Demonstrating the Engineering Feasibility of Interstellar Travel(British Interplanetary Society, 2015), ISBN 978-0950659701

    2015

  31. [38]

    G.Marx,InterstellarVehiclePropelledByTerrestrialLaserBeam,Nature211,22-23(1966), https://doi.org/10.1038/211022a0

    1966 doi

  32. [39]

    J. L. Redding,Interstellar Vehicle propelled by Terrestrial Laser Beam, Nature213, 588-589 (1967), https://doi.org/10.1038/213588a0

    1967 doi

  33. [40]

    Lubin,A Roadmap to Interstellar Flight, Journal of the British Interplanetary Society69, 40-72 (2016) [arXiv:1604.01356 [astro-ph.EP]]

    P. Lubin,A Roadmap to Interstellar Flight, Journal of the British Interplanetary Society69, 40-72 (2016) [arXiv:1604.01356 [astro-ph.EP]]

    2016 arXiv

  34. [41]

    P.Lubin,ThePathtoTransformationalSpaceExploration(WorldScientificPublishingCom- pany, 2022), ISBN 978-981-12-4903-7, 978-981-12-4828-3, https://doi.org/10.1142/11918

    2022 doi

  35. [42]

    K. L. G. Parkin,The Breakthrough Starshot system model, Acta Astronautica152, 370-384 (2018), https://doi.org/10.1016/j.actaastro.2018.08.035 [arXiv:1805.01306 [astro-ph.IM]]

    2018 doi arXiv

  36. [43]

    J. Y. Lin, C. M. de Sterke, O. Ilic and B. T. Kuhlmey,Photonic Lightsails: Fast and Stable Propulsion for Interstellar Travel, https://doi.org/10.48550/arXiv.2502.17828 [arXiv:2502.17828 [astro-ph.IM]]

    doi arXiv

  37. [44]

    T. M. Eubanks, J. Schneider, B. Bills, et al.,Science from the In Situ Exploration of the Prox- ima Centauri System, https://doi.org/10.48550/arXiv.2604.20182 [arXiv:2604.20182 [astro- ph.IM]]

    doi arXiv

  38. [45]

    Bambi, A

    C. Bambi, A. D. Dolgov and A. A. Petrov,Black holes as antimatter factories, JCAP09, 013 (2009) https://doi.org/10.1088/1475-7516/2009/09/013 [arXiv:0806.3440 [astro-ph]]

    2009 doi arXiv

  39. [46]

    Bambi, D

    C. Bambi, D. Malafarina and N. Tsukamoto,Note on the effect of a massive accre- tion disk in the measurements of black hole spins, Phys. Rev. D89, 127302 (2014) https://doi.org/10.1103/PhysRevD.89.127302 [arXiv:1406.2181 [gr-qc]]

    2014 doi arXiv

  40. [47]

    L. Gao, C. Bambi, Y. Fan, T. Mirzaev, A. Nosirov and A. Santangelo,Testing Black Holes with Interstellar Missions: I. Orbiting Probes, https://doi.org/10.48550/arXiv.2605.19176 [arXiv:2605.19176 [gr-qc]]. 11 A Space Mission to Earth’s Nearest Black HoleCosimo Bambi

    doi arXiv

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