Astrobiology16- Page

Cartoon illustration of the hybrid models. The difference between HM-U and HM-C is in the first step, where the initial planet masses and radii are drawn (HMC draws clustered initial

Proposed formation pathways of biorelevant molecules (red arrows) in hydrogen cyanide (HCN)-containing interstellar ices and their role as precursors to biorelevant molecules such as amino acids and nucleobases. In prebiotic

Endor (source) – Starwars.com Giant planets in the habitable zone may host exomoons with conditions conducive to life. In this paper we describe a method by which the Habitable Worlds

Color-magnitude diagram for nearby stars (within 100 pc) showing the local main sequence in MG vs BP − RP. The background density map is constructed from the Gaia Catalogue of

The different Solar System bodies and exoplanets this chapter focuses on, and associated missions. Those with a strong PlanetS involvement are shown with an asterisk. — astro-ph.EP Understanding the climates

Composite image of the field-of-view mapped in the Horsehead nebula (Barnard 33). Left: The Horsehead nebula and the adjacent H II region IC 434 imaged by Euclid Early Release Observations

Time series of RV and activity indicators. Panel (a): RV time series. Panel (b): GLS periodogram related to the RV time series. We see two prominent peaks in correspondence with

Spectra of targets meeting our selection criteria for further analysis (P/C>0.2 and H218O SNR>2), between 22.7 and 24.2 µm, along with best-fit 3-component water models (blue; see Table 1),