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CSDA Menu CSDA Commercial Data Commercial Datasets Commercial Satellite Data Explorer Satellite Data Evaluation CSDA Vendors Airbus BlackSky Capella Space GeoOptics GHGSat ICEYE Vantor Planet PlanetiQ Polar Geospatial Center Satellogic
Our planet rests inside a magnetic cocoon filled with plasma – but it’s not always peaceful and quiet. Activity from the Sun can send waves through this space, and some
The formation mechanism of the lower haze. Cosmic dust entering from space is incorporated into sulfuric acid clouds. As sulfuric acid evaporates at the cloud base, the dust particles remain
Graphical abstract The PAH-water (PAH = polycyclic aromatic hydrocarbon) interactions occur in interstellar ice grains and in atmospheres of planets and can serve as models for the interaction between water
Summary: Orpheus is a Mars hopper mission concept to explore volcanic fissures and pit/cave vents in Cerberus Fossae that experienced recent eruptions and may still be active, to search for
An artist’s concept illustrates a dusty planet-forming disk — NASA Meteorites are classified as either non-carbonaceous- (NC) or carbonaceous (CC), representing bodies that likely formed in the inner- or outer
Details of the interior models of Uranus and Neptune. Top: Illustration of the three-layer internal structure model assumed. Both the envelope and mantle contain hydrogen, helium, ices, and rocks, with
Number of light curves for stars in LOPS2 classified per TESS sector. The entire bin height indicates all light curves for a given sector, where those with a dominant instrumental
Best-fit white light (5.06–10.55 µm) curves of HD 3167 b’s secondary eclipse from our SPARTA (blue), Eureka! (red), and exoTEDRF (green) reductions. (Top) Binned raw white light fluxes. The best-fit
NASA/JPL-Caltech/IPAC/Hora et al. An observation made by NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) shows the chemical signatures of water ice (shown






