(left) Electromagnetic model showing the suppression of AKR and Earth transmitters on the far side of the Moon (Bassett et al. 2020). (Right) Eight candidate sites on the farside identified
(left) Electromagnetic model showing the suppression of AKR and Earth transmitters on the far side of the Moon (Bassett et al. 2020). (Right) Eight candidate sites on the farside identified
The Viking 1 Lander sampling arm created a number of deep trenches as part of the surface composition and biology experiments on Mars. The digging tool on the sampling arm
Model prediction on a test sequence from the semi-synthetic TW Hya dataset. The red circle indicates the true position of the injected planet in each frame. In the first frame,
Upper panel: top view of one of the non-porous (npASW) (left) and porous (pASW) ice models. Each periodic surface contains 500 water molecules. Lower panel: altitude plot relative to the
A single MIRI imaging integration of LTT 3780 b, taken from Observation 15, cut from 90 to 165 pixels in each direction of the whole frame. Shown in red is
MATRIX injection-and-recovery experiment conducted to establish the detection limits using the ten TESS sectors described in Sect. 3.1. We explored a total of 18000 different scenarios, where each pixel evaluated
Ceres’s temperature evolution drives major interior events. – Depending on the extent of internal heating, a mid-sized (~500- to 1000-km radius) icy body such as Ceres may undergo differentiation and
Best-fitting relative brightness distribution of the Sun for each of the 23 chunks listed in Tab. 1 and shown in Fig. 1. The color scale depicts the logarithm of the
(LEFT) Combined 130 s F350LP image of 3I/ATLAS showing diffuse asymmetric emission to the north west. (RIGHT) Same image contoured, with scale bar and direction arrows shown. The yellow and
Some hypersaline environments in Latin America. A-B. Salt crust and the famous mirage in the Salar de Uyuni, Bolivia. Source: Photos taken by Nicole Jimeno. C-D. Salt formation in the