Planetary and Space Science
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| Planetary and Space Science | |
|---|---|
| Title | Planetary and Space Science |
| Discipline | Astronomy; Geophysics; Astrophysics |
| Publisher | Elsevier |
| Country | Netherlands |
| Established | 1959 |
| Frequency | Monthly |
| Issn | 0032-0633 |
Planetary and Space Science Planetary and Space Science is a multidisciplinary field encompassing the study of Mars, Venus, Mercury, Jupiter, Saturn, Uranus, Neptune, Pluto, Moon, Io, Europa, Ganymede, Callisto, Enceladus, Titan, Ceres, Vesta, Comet 67P/Churyumov–Gerasimenko, Halley's Comet, Sun and extrasolar systems through observational, experimental, theoretical, and computational approaches. Researchers draw on techniques from NASA, European Space Agency, Roscosmos, China National Space Administration, Indian Space Research Organisation, Japan Aerospace Exploration Agency, SpaceX, Blue Origin, Arianespace and national observatories including Mauna Kea Observatories, Palomar Observatory, Green Bank Observatory and Arecibo Observatory. The field intersects with missions such as Voyager program, Pioneer program, Galileo, Cassini–Huygens, Magellan, MESSENGER, Mariner program, Viking program, Mars Reconnaissance Orbiter, Curiosity, Perseverance, InSight, Phoenix, Viking 1, Viking 2, Luna programme, Chang'e 4, Chandrayaan-2, Hayabusa2, Osiris-REx, New Horizons, Juno and telescopes like Hubble Space Telescope, James Webb Space Telescope, Spitzer Space Telescope, Kepler space telescope, Transiting Exoplanet Survey Satellite, Chandra X-ray Observatory.
Overview and Scope
Planetary and space science integrates studies of Solar System bodies, exoplanet populations, interplanetary media and stellar influences using data from planetary exploration, ground-based facilities and space telescopes. Core institutions include Royal Astronomical Society, American Astronomical Society, European Southern Observatory, Max Planck Institute for Solar System Research, Smithsonian Astrophysical Observatory, Jet Propulsion Laboratory, Caltech, MIT, Stanford University and University of Cambridge. Research themes arise from historic programs like Mariner 9, Venera program, Apollo program, Surveyor program and policy frameworks such as Outer Space Treaty guiding United Nations Office for Outer Space Affairs collaborations. Funding and peer review derive from agencies like National Science Foundation, European Research Council, Russian Academy of Sciences and foundations including Simons Foundation.
Planetary Science
Planetary science addresses formation and evolution of protoplanetary disk, planetary differentiation, core–mantle boundary, plate tectonics on Earth, global magnetic fields observed at Mercury, Moon and Ganymede, and volatile cycles on Mars and Titan. Major subfields examine impact cratering (e.g. studies referencing Chicxulub crater), volcanism on Io and Olympus Mons, regolith processes at Lunar Reconnaissance Orbiter, and atmospheres of Venus and Titan with missions like Venus Express and Cassini–Huygens. Isotope geochemistry links laboratories such as Lawrence Livermore National Laboratory, Oak Ridge National Laboratory, Scripps Institution of Oceanography and museum collections like Smithsonian National Air and Space Museum for meteoritic studies including Allende (meteorite), Murchison meteorite and Nakhla meteorite.
Solar and Stellar Physics
Solar and stellar physics probes solar wind, heliosphere, stellar magnetic dynamos, flares, coronal heating and activity cycles observed by Solar and Heliospheric Observatory, Parker Solar Probe, Solar Dynamics Observatory, Hinode, Yohkoh, SOHO and ground networks like Global Oscillation Network Group. Comparative stellar studies use facilities such as Kepler space telescope and Gaia to map exoplanet host stars and stellar evolution across clusters like Pleiades, Hyades, and Globular Cluster Messier 13. Theoretical frameworks reference work by Subrahmanyan Chandrasekhar, Eugene Parker, Hans Alfvén, Edwin Salpeter, Fred Hoyle and institutions like Princeton University and University of Chicago.
Space Environment and Space Weather
Space weather research focuses on magnetospheric dynamics at Earth, Jupiter and Saturn using missions Cluster, THEMIS, MMS, JUICE and ground arrays like SuperDARN, Low Frequency Array and Very Large Array. Studies of radiation belts invoke data from Van Allen Probes, GOES (satellite), ACE, Wind and national centers including NOAA and UK Met Office. Phenomena such as geomagnetic storms, coronal mass ejections, solar energetic particles and aurorae tie into infrastructure concerns addressed by International Civil Aviation Organization, Federal Aviation Administration, European Union Agency for the Space Programme and standards bodies.
Exploration and Instrumentation
Exploration and instrumentation cover landers, rovers, orbiters and remote sensing payloads: Alpha Particle X-ray Spectrometer, Mössbauer spectrometer, ChemCam, SHERLOC, SAM (Sample Analysis at Mars), Mastcam-Z, Synthetic Aperture Radar on Magellan, HiRISE on Mars Reconnaissance Orbiter, RADAR on Cassini–Huygens, and sample-return architectures exemplified by Hayabusa, Hayabusa2, OSIRIS-REx and planned Mars Sample Return. Engineering and project teams at Lockheed Martin, Northrop Grumman, Boeing, Thales Alenia Space, Airbus Defence and Space, ISRO and research labs develop instrumentation standards and calibration protocols.
Theoretical Models and Computational Methods
Theoretical and computational methods employ magnetohydrodynamics, radiative transfer, N-body simulations, Monte Carlo techniques, data assimilation and inverse methods implemented on high-performance computing centers like NERSC, PRACE, TACC and supercomputers such as Summit (supercomputer), Fugaku. Modeling efforts link groups at NASA Ames Research Center, European Space Agency Science Directorate, Max Planck Institutes, Harvard–Smithsonian Center for Astrophysics and Los Alamos National Laboratory to produce predictive frameworks for planetary interiors, climate, orbital dynamics, tidal interactions, disk evolution and atmospheric escape. Prominent modeling codes originate from collaborations involving MIT, Caltech, University of Colorado Boulder, University of Oxford, University of California, Berkeley and international consortia coordinating through conferences like American Geophysical Union, European Geosciences Union, International Astronomical Union and journals managed by Elsevier, Springer Nature, Oxford University Press.