The emirates Mars mission

HES Amiri, D Brain, O Sharaf, P Withnell… - Space Science …, 2022 - Springer
Abstract The Emirates Mars Mission (EMM) was launched to Mars in the summer of 2020,
and is the first interplanetary spacecraft mission undertaken by the United Arab Emirates …

The emirates Mars ultraviolet spectrometer (EMUS) for the EMM mission

GM Holsclaw, J Deighan, H Almatroushi… - Space Science …, 2021 - Springer
Abstract The Emirates Mars Mission (EMM) Hope probe was launched on 20 July 2020 at
01: 58 GST (Gulf Standard Time) and entered orbit around Mars on 9 Feb 2021 at 19: 42 …

Atmospheric escape processes and planetary atmospheric evolution

G Gronoff, P Arras, S Baraka, JM Bell… - Journal of …, 2020 - Wiley Online Library
The habitability of the surface of any planet is determined by a complex evolution of its
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …

Ion energization and escape on Mars and Venus

E Dubinin, M Fraenz, A Fedorov, R Lundin… - The plasma environment …, 2012 - Springer
Mars and Venus do not have a global magnetic field and as a result solar wind interacts
directly with their ionospheres and upper atmospheres. Neutral atoms ionized by solar UV …

Planetary evolution with atmospheric photoevaporation-II. Fitting the slope of the radius valley by combining boil-off and XUV-driven escape

L Affolter, C Mordasini, AV Oza, D Kubyshkina… - Astronomy & …, 2023 - aanda.org
Context. Observations by the Kepler satellite have revealed a gap between larger sub-
Neptunes and smaller super-Earths that atmospheric escape models had predicted as an …

Photochemical escape of oxygen from Mars: A comparison of the exobase approximation to a Monte Carlo method

JL Fox, AB Hać - Icarus, 2009 - Elsevier
The non-thermal escape of neutral O atoms from Mars at the current epoch is largely due to
dissociative recombination of O2+: There are five energetically allowed channels of this …

Heating efficiency in hydrogen-dominated upper atmospheres

VI Shematovich, DE Ionov, H Lammer - Astronomy & Astrophysics, 2014 - aanda.org
Context. The heating efficiency η hν is defined as the ratio of the net local gas-heating rate to
the rate of stellar radiative energy absorption. It plays an important role in thermal-escape …

Formation and evolution of protoatmospheres

H Massol, K Hamano, F Tian, M Ikoma, Y Abe… - Space Science …, 2016 - Springer
The origin and evolution of planetary protoatmospheres in relation to the protoplanetary disk
is discussed. The initial atmospheres of planets can mainly be related via two formation …

Airglow and aurora in the Martian atmosphere: contributions by the Mars Express and ExoMars TGO missions

F González-Galindo, JC Gérard, L Soret… - Space Science …, 2024 - Springer
The study of atmospheric emissions from orbit to probe the middle and upper atmosphere of
Mars, which started with the Mariner missions, is living a golden era thanks to the European …

Thermally driven atmospheric escape: Transition from hydrodynamic to Jeans escape

AN Volkov, RE Johnson, OJ Tucker… - The Astrophysical …, 2011 - iopscience.iop.org
Thermally driven escape from planetary atmospheres changes in nature from an organized
outflow (hydrodynamic escape) to escape on a molecule-by-molecule basis (Jeans escape) …