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

cris.virtual.author-orcid0000-0002-2160-8782
cris.virtual.author-orcid0000-0002-9355-5165
cris.virtual.author-orcid0000-0003-4269-3311
cris.virtualsource.author-orcid558d5c26-a12b-4181-8161-fa58a8a267ef
cris.virtualsource.author-orcidae0b1c52-3484-4f76-9d81-edd1f9d1e9a4
cris.virtualsource.author-orcid9b56f22e-0983-4b84-b800-fb636eff882e
cris.virtualsource.author-orcid475bfbaf-a55c-46d3-9e40-35ed815e4ddf
cris.virtualsource.author-orcid03da1793-6b6a-443b-8822-84fec43bea7f
datacite.rightsopen.access
dc.contributor.authorAugust, P. C.
dc.contributor.authorBuchhave, L. A.
dc.contributor.authorDiamond-Lowe, H.
dc.contributor.authorMendonça, J. M.
dc.contributor.authorGressier, A.
dc.contributor.authorRathcke, A. D.
dc.contributor.authorAllen, N. H.
dc.contributor.authorFortune, M.
dc.contributor.authorJones, K. D.
dc.contributor.authorMeier Valdés, E. A.
dc.contributor.authorDemory, B.-O.
dc.contributor.authorEspinoza, N.
dc.contributor.authorFisher, C. E.
dc.contributor.authorGibson, N. P.
dc.contributor.authorHeng, Kevin
dc.contributor.authorHoeijmakers, J.
dc.contributor.authorHooton, M. J.
dc.contributor.authorKitzmann, Daniel
dc.contributor.authorPrinoth, B.
dc.contributor.authorEastman, J. D.
dc.contributor.authorBarnes, R.
dc.date.accessioned2025-05-13T07:03:51Z
dc.date.available2025-05-13T07:03:51Z
dc.date.issued2025-03
dc.description.abstractContext. 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.
dc.description.sponsorshipPhysics Institute
dc.description.sponsorshipARTORG Center - Artificial Intelligence in Medical Image Computing
dc.description.sponsorshipCenter for Space and Habitability (CSH)
dc.description.sponsorshipSpace Research and Planetology Physics - Planetary Evolution
dc.description.sponsorshipARTORG Center for Biomedical Engineering Research
dc.identifier.doi10.48620/87992
dc.identifier.publisherDOI10.1051/0004-6361/202452611
dc.identifier.urihttps://boris-portal.unibe.ch/handle/20.500.12422/210881
dc.language.isoen
dc.publisherEDP Sciences
dc.relation.ispartofAstronomy & Astrophysics
dc.relation.issn0004-6361
dc.relation.issn1432-0746
dc.relation.issn0004-6361
dc.titleHot Rocks Survey I: A possible shallow eclipse for LHS 1478 b
dc.typearticle
dspace.entity.typePublication
dspace.file.typetext
oaire.citation.volume695
oairecerif.author.affiliationCenter for Space and Habitability (CSH)
oairecerif.author.affiliationCenter for Space and Habitability (CSH)
oairecerif.author.affiliationPhysics Institute
oairecerif.author.affiliationARTORG Center - Artificial Intelligence in Medical Image Computing
oairecerif.author.affiliationSpace Research and Planetology Physics - Planetary Evolution
oairecerif.author.affiliation2Center for Space and Habitability (CSH) - ESP ExoClimes
oairecerif.author.affiliation2Center for Space and Habitability (CSH)
oairecerif.author.affiliation2ARTORG Center for Biomedical Engineering Research
oairecerif.author.affiliation2Physics Institute
unibe.additional.sponsorshipARTORG Center for Biomedical Engineering Research
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unibe.description.ispublishedpub
unibe.refereedtrue
unibe.subtype.articlejournal

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