Planet Venus: Japan’s Venus Climate Orbiter Ultraviolet View December 23, 2016 – JAXA Context: Planets in the HZ can have dense atmospheres affecting their rotations. Over time, the rotation tends

The different views of B3LYP-D3(BJ)/6- 311++G(d,p) level optimized geometric structures for 9- iminofluorene (left) and benzophenone imine (right). The arrow shows C9 position of iminofluorene. — astro-ph.GA Interstellar detections of

TESS target pixel file images of TOI-2094 (LEFT) and TOI-7166 (RIGHT). The red circles are sources identified by Gaia DR3 catalogue (Gaia Collaboration et al. 2016, 2023), labelled with numbers

Structures and relative energy levels of cis-HNSO (left, as the ground state), trans-HNSO (right, at 3.7 kcal/mol), and the transition state (middle, at 14.5 kcal/mol); energy values were derived by

Plot of the Habitable Zone (HZ) completeness as a function of host star luminosity (in units of Solar luminosity) and distance (in parsecs). Here the AYO results are on the