ISM abundances Cosmology observations Asteroseismology Gamma rays general Stratigraphy Star formation Magnetic reconnection Stars magnetic field Satellite Methods observational Jezero crater Stars fundamental parameters Hydrodynamics Submillimeter ISM Stars oscillations Galaxies clusters general Methods statistical MAVEN Galaxies clusters intracluster medium Polarization ISM clouds Magnetic fields Black hole physics Cherenkov Telescope Array X-rays general Surveys Accretion disks Sedimentology Interstellar medium Instabilities Dust Cosmological parameters Stars activity Stars evolution Astrophysics - High Energy Astrophysical Phenomena Astrochemistry X-rays binaries Astrophysics - Earth and Planetary Astrophysics Catalogs Cosmic background radiation polarization Perseverance Magnetosphere Spectroscopy Sensitivity MSL Dark matter Galaxies formation Physics - Space Physics Turbulence Sun magnetic fields Methods data analysis Delta Accretion Techniques polarimetric Cosmic rays Stars low-mass Solar wind Stars rotation Galaxies active Astrophysics - Instrumentation and Methods for Astrophysics Gale crater Radiative transfer Galaxies Galaxies high-redshift Seismology ISM molecules Stars neutron Large-scale structure of Universe Ionosphere Stars formation Galaxies star formation Techniques photometric Extinction Astrophysics Galaxies evolution Instrumentation Magnetohydrodynamics MHD Astrophysics - Astrophysics of Galaxies Stars interiors Mars Reionization Infrared ISM Observatory Accretion discs Methods numerical Astrophysics - Solar and Stellar Astrophysics Galaxies starburst Stars solar-type Plasmas ISM jets and outflows Cosmic background radiation Galaxies ISM Mars 2020 Stars protostars X-rays galaxies clusters Galaxy Planetary systems Cosmological model Techniques spectroscopic Protoplanetary disks