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Hot Rocks Survey I : A possible shallow eclipse for LHS 1478 b

August, P. C. ; Buchhave, L. A. ; Diamond-Lowe, H. ; Mendonça, J. M. ; Gressier, A. ; Rathcke, A. D. ; Allen, N. H. ; Fortune, M. ; Jones, K. D. and Meier Valdés, E. A. , et al. (2025) In Astronomy and Astrophysics 695.
Abstract

Context. M-dwarf systems offer an opportunity to study terrestrial exoplanetary atmospheres due to their small size and cool temperatures. However, the extreme conditions imposed by these host stars raise a question about whether their close-in rocky planets are able to retain any atmosphere at all. Aims. The Hot Rocks Survey aims to answer this question by targeting nine different M-dwarf rocky planets spanning a range of planetary and stellar properties. Of these, LHS 1478 b orbits an M3-type star, has an equilibrium temperature of Teq = 585 K, and receives 21 times Earth's instellation. Methods. We observed two secondary eclipses of LHS 1478 b using photometric imaging at 15 μm using the Mid-Infrared Instrument on the... (More)

Context. M-dwarf systems offer an opportunity to study terrestrial exoplanetary atmospheres due to their small size and cool temperatures. However, the extreme conditions imposed by these host stars raise a question about whether their close-in rocky planets are able to retain any atmosphere at all. Aims. The Hot Rocks Survey aims to answer this question by targeting nine different M-dwarf rocky planets spanning a range of planetary and stellar properties. Of these, LHS 1478 b orbits an M3-type star, has an equilibrium temperature of Teq = 585 K, and receives 21 times Earth's instellation. Methods. We observed two secondary eclipses of LHS 1478 b using photometric imaging at 15 μm using the Mid-Infrared Instrument on the James Webb Space Telescope (JWST MIRI) to measure thermal emission from the dayside of the planet. We compared these values to atmospheric models to evaluate potential heat transport and CO2 absorption signatures. Results. We find that a secondary eclipse depth of 138 ± 53 ppm at the expected time for a circular orbit is preferred over a null model at 2.8σ, a moderate detection, though dynamical models do favour a non-eccentric orbit for this planet. The second observation results in a non-detection due to significantly larger unexplained systematics. Based on the first observation alone, we can reject the null hypothesis of the dark (zero Bond albedo) no atmosphere bare rock model with a confidence level of 3.3σ, though for AB = 0.2 the significance decreases to 2.1σ. The tentative secondary eclipse depth is consistent with the majority of the atmospheric scenarios we considered, spanning CO2-rich atmospheres with surface pressures from 0.1 to 10 bar. However, we stress that the two observations from our programme do not yield consistent results, and more observations are needed to verify our findings. The Hot Rocks Survey serves as a relevant primer for future endeavours such as the Director's Discretionary Time (DDT) Rocky Worlds programme.

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publishing date
type
Contribution to journal
publication status
published
subject
keywords
Planets and satellites: atmospheres, Planets and satellites: terrestrial planets, Techniques: photometric
in
Astronomy and Astrophysics
volume
695
article number
A171
publisher
EDP Sciences
external identifiers
  • scopus:105000381450
ISSN
0004-6361
DOI
10.1051/0004-6361/202452611
language
English
LU publication?
yes
id
74253e27-8293-491e-a138-5cbded71fe54
date added to LUP
2026-01-09 14:33:01
date last changed
2026-01-09 14:34:07
@article{74253e27-8293-491e-a138-5cbded71fe54,
  abstract     = {{<p>Context. M-dwarf systems offer an opportunity to study terrestrial exoplanetary atmospheres due to their small size and cool temperatures. However, the extreme conditions imposed by these host stars raise a question about whether their close-in rocky planets are able to retain any atmosphere at all. Aims. The Hot Rocks Survey aims to answer this question by targeting nine different M-dwarf rocky planets spanning a range of planetary and stellar properties. Of these, LHS 1478 b orbits an M3-type star, has an equilibrium temperature of T<sub>eq</sub> = 585 K, and receives 21 times Earth's instellation. Methods. We observed two secondary eclipses of LHS 1478 b using photometric imaging at 15 μm using the Mid-Infrared Instrument on the James Webb Space Telescope (JWST MIRI) to measure thermal emission from the dayside of the planet. We compared these values to atmospheric models to evaluate potential heat transport and CO<sub>2</sub> absorption signatures. Results. We find that a secondary eclipse depth of 138 ± 53 ppm at the expected time for a circular orbit is preferred over a null model at 2.8σ, a moderate detection, though dynamical models do favour a non-eccentric orbit for this planet. The second observation results in a non-detection due to significantly larger unexplained systematics. Based on the first observation alone, we can reject the null hypothesis of the dark (zero Bond albedo) no atmosphere bare rock model with a confidence level of 3.3σ, though for A<sub>B</sub> = 0.2 the significance decreases to 2.1σ. The tentative secondary eclipse depth is consistent with the majority of the atmospheric scenarios we considered, spanning CO<sub>2</sub>-rich atmospheres with surface pressures from 0.1 to 10 bar. However, we stress that the two observations from our programme do not yield consistent results, and more observations are needed to verify our findings. The Hot Rocks Survey serves as a relevant primer for future endeavours such as the Director's Discretionary Time (DDT) Rocky Worlds programme.</p>}},
  author       = {{August, P. C. and Buchhave, L. A. and Diamond-Lowe, H. and Mendonça, J. M. and Gressier, A. and Rathcke, A. D. and Allen, N. H. and Fortune, M. and Jones, K. D. and Meier Valdés, E. A. and Demory, B. O. and Espinoza, N. and Fisher, C. E. and Gibson, N. P. and Heng, K. and Hoeijmakers, J. and Hooton, M. J. and Kitzmann, D. and Prinoth, B. and Eastman, J. D. and Barnes, R.}},
  issn         = {{0004-6361}},
  keywords     = {{Planets and satellites: atmospheres; Planets and satellites: terrestrial planets; Techniques: photometric}},
  language     = {{eng}},
  publisher    = {{EDP Sciences}},
  series       = {{Astronomy and Astrophysics}},
  title        = {{Hot Rocks Survey I : A possible shallow eclipse for LHS 1478 b}},
  url          = {{http://dx.doi.org/10.1051/0004-6361/202452611}},
  doi          = {{10.1051/0004-6361/202452611}},
  volume       = {{695}},
  year         = {{2025}},
}