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Distances, Luminosities, and Temperatures of the Coldest Known Substellar Objects

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

The coolest known brown dwarfs are our best analogs to extrasolar gas-giant planets. The prolific detections of such cold substellar objects in the past two years has spurred intensive followup, but the lack of accurate distances is a key gap in our understanding. We present a large sample of precise distances based on homogeneous mid-infrared astrometry that robustly establish absolute fluxes, luminosities, and temperatures. The coolest brown dwarfs have temperatures of 400-450 K and masses ~5-20 times that of Jupiter, showing they bridge the gap between hotter brown dwarfs and gas-giant planets. At these extremes, spectral energy distributions no longer follow a simple correspondence with temperature, suggesting an increasing role of other physical parameters such as surface gravity, vertical mixing, clouds, and metallicity.

fields

astro-ph.EP 2

years

2026 2

verdicts

UNVERDICTED 2

representative citing papers

Ultra-Precise Astrometric Search for Exoplanets with SKA-VLBI

astro-ph.EP · 2026-06-23 · unverdicted · novelty 4.0

SKA-VLBI is projected to deliver an order-of-magnitude gain in astrometric precision, enabling detection of thousands of exoplanets around ultra-cool dwarfs, M dwarfs and young stars plus dynamical masses when companions are also imaged.

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Showing 2 of 2 citing papers.

  • $^{13}$CO and potential variability in $\beta$ Pictoris b with GRAVITY+ astro-ph.EP · 2026-06-10 · unverdicted · none · ref 39 · internal anchor

    GRAVITY+ observations yield a 12CO/13CO ratio of 91^{+24}_{-17} in β Pictoris b consistent with solar/ISM values and a tentative 1.4% atmospheric variability amplitude.

  • Ultra-Precise Astrometric Search for Exoplanets with SKA-VLBI astro-ph.EP · 2026-06-23 · unverdicted · none · ref 28 · internal anchor

    SKA-VLBI is projected to deliver an order-of-magnitude gain in astrometric precision, enabling detection of thousands of exoplanets around ultra-cool dwarfs, M dwarfs and young stars plus dynamical masses when companions are also imaged.