ID: ESP_066552_1215, date: 7 October 2020,altitude: 247 km,NASA/JPL-Caltech/University of Arizonalarger image This HiRISE image shows a deposit draping the surface like a blanket. The deposit is eroding away, and near

The explosion left behind an interstellar gas-and-dust cloud rich in silicon (gray), sulfur (yellow) and argon (purple). Credit: Keck Observatory/Adam Makarenko Massive stars have a layered structure, similar to an

GC content, total number and their frequencies of PQS in H. volcanii genome. (A) Schematic presentation of a G-quartet (left) and a G-quadruplex (right). (B) Total PQS counts, percentage of

Growth tracks of a single planet injected at r = 3 AU and t = 104 yr. In the irradiated case (left), this results in the formation of a super-Earth

Altitude integrated joule heating for scale factors 1, 5, and 10. Gradient uses the same maximum value for visible demonstration of the changes between the images — astro-ph.EP Identifying Earth-like

The distribution of accretion parameters relative to steady state derived from the posteriors of the MCMC tests, separated based on the dominant atmospheric species. To compare accretion phases, we have

3D hydrodynamic simulation of atmospheric escape from Ref. 8, for a system similar to HAT-P-67 b. Figure 2a shows the gas density. The star is in the center of the