A Revised Density Estimate for the Largest Known Exoplanet, HAT-P-67 b
Low-density ( ρ _p < 0.1 g cm ^−3 ) hot Saturns are expected to quickly (<100 Myr) lose their atmospheres owing to stellar irradiation, explaining their rarity. HAT-P-67 b seems to be an exception, with ρ _p < 0.09 g cm ^−3 and maintaining its atmosphere to well after 1 Gyr. We present a photometr...
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| Principais autores: | , , , , , , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
IOP Publishing
2025-01-01
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| coleção: | The Astronomical Journal |
| Assuntos: | |
| Acesso em linha: | https://doi.org/10.3847/1538-3881/adcec9 |
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