Astrobiology50- Page

Hyperspectral maps of RR5-70-1. (a) Photograph of the RR5-70-1 original core. Dotted white outline shows cut sample region used for neutron computed tomographic scan (i.e., Figure 8a). (b) Hyperspectral image

Current and forthcoming constraints on radio line broadcasts in M31 (left) and three example Virgo cluster ellipticals (right), assuming that all broadcasts in each galaxy have the same EIRP ℓ.

Graph of the semimajor axis and eccentricity of the final terrestrial planets in the simulations of Table 1. Note that the majority of the planets formed or reached their final

Fraction of atmosphere retained 1 Gyr after a hypothetical Moonforming impact with 𝑓esc = 0.01 and 𝐷max = 100 km, as a function of the initial atmospheric mass (𝑚atm0). Filled

In the large graph, simulated matched-filter S/N over 1000 hours as a function of R, dark current, and read noise, for a modern exo-Earth orbiting a Sun-like star as observed

Number of stars capable of hosting observers (amongst a sample of 106) as a function of time. The darkest track assumes that all stars are equally capable of hosting life

Geographic map of vent field locations Map data 2025 Google. — Molecular Ecology Genetic bottlenecks are evolutionary events that reduce the effective size and diversity of natural populations, often limiting

ETI broadcasts of a galaxy over its history form a population described by distributions (left). Surveys, and observations within the surveys, select subsets of the positions, times, and frequencies (and

Extensions to the HZ (the orange stripe) as a function of distance between the planet and its host star (horizontal axis), and the mass of the Main Sequence host (vertical