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Candor Chasma in central Valles Marineris — NASA HiRISE Candor Chasma in central Valles Marineris is filled with light-toned layered deposits thought to be sandstones, perhaps formed in an ancient

Illustration of the various probabilities discussed. The variable x may refer to any of the physical constants α, β, γ etc., with the others integrated over. The dashed lines indicate

The architectures of the systems with both small planets and cold Jupiters considered in this work and ordered according to increasing semi-major axis of the innermost planet (from bottom to

MUSE and NIRCam images of d203-504 environment. Left: MUSE NFM composite image of both d203-506 (bottom left) and d203-504 (top). Red: the (λ8727˚A) map showing disk contributions from both

True colour image of a cloud-free Ocean planet at α = 90◦with different surface wind speed maps. In the first row, we use a constant wind speed and notice the