Astrobiology98- Page

The top and lower left panels show the integrated intensity map and the intensity-weighted velocity for EG. The top and lower right panels show the same for GN. We only

a, Orbital context image with the rover traverse overlain in white. White line and arrows show the direction of the rover traverse from the southern contact between the Margin Unit

Mineralogical map of Jezero crater explored by the Perseverance rover. This mineral map was created from near-infrared (1-2.6 µm) CRISM imagery (Parente et al., 2021) using recently developed technologies (Itoh

(a) “Small” grain core assembled up of 1000 carbon atoms; (b) cross-section of a “small” grain core; (c) ’large’ grain core assembled up of 10000 carbon atoms; (d) cross-section of

Position on the Gaia CMD diagram of the stars that experienced a close encounter with 3I/ATLAS, with spectral types indicated in the legend that comes from O. L. Creevey et

Left panel: IFU transmission map into the 7 fibers for single orientation, with the trajectory of Proxima b overlaid on top. Right panel: IFU transmission combining 2 exposures with a

Example Bioverse simulation of a survey to characterize Earth-sized planets in the HZ. This simulation used an 8m diameter telescope observing at λ= 550nm. This figure shows all rocky planets

Earth-like and super Earth planet candidates from (5) are shown in the effective temperature – instellation flux plane. Conservative and optimistic Habitable zones as defined in (5) are shown as

Schematic of the TRAPPIST-1 planetary system. The seven known planets are shown orbiting the central star. The semi-transparent green annulus marks the optimistic habitable zone, which contains planets e, f,