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Telescope observations, star catalogs, exoplanet surveys, galaxy morphology, gravitational waves, spectroscopy
2,943 datasets
NASA's VIRTIS instrument telemetry data from the Rosetta spacecraft's orbit of comet 67P. The dataset contains digital numbers (DN) from the EXTENSION 3 MTP031 phase, which occurred from 2016-06-29 to 2016-07-27. The data was last updated on 2026-03-13.
The Ulysses spacecraft's GAS experiment sky maps show count rates of interstellar helium particles and celestial UV intensities. The dataset is produced by the National Aeronautics and Space Administration. The data was last updated on 2026-03-13.
Corrected and resampled calibrated data from the RPCICA instrument on the Rosetta spacecraft during its second mission extension. Measurements likely contain time-series data of solar wind interaction with the atmosphere of comet 67P/Churyumov-Gerasimenko. The dataset is provided by the National Aeronautics and Space Administration and was last updated on March 13, 2026.
MESSENGER Neutron Spectrometer calibrated data records contain neutron spectra emitted from Mercury's surface in the energy range from 0.01 eV to 7 MeV. The data set includes five products: raw neutron spectra, NS counter data, galactic cosmic ray spectra, engineering data, and gamma-ray burst data. Version 2.0 was published by NASA and supersedes version 1.
Photometric magnitude measurements of comet 1P/Halley submitted to the International Halley Watch Photometry and Polarimetry Network. Both broadband and narrowband magnitudes are included, with filter parameters for each measurement. This second version includes corrections to known errata and a combined chronological table.
NASA's Rosetta spacecraft VIRTIS instrument telemetry data contains digital numbers (DN) from the PRELANDING MTP009 phase near comet 67P. The data covers a specific period from October 24, 2014, to November 22, 2014. The dataset was last updated on March 13, 2026.
NASA's Planetary Data System archives calibrated data from the SESAME instrument on the ROSETTA Lander, acquired during the Surface Science and Dust Detection (SDL) phase. The primary target is comet 67P/Churyumov-Gerasimenko. This dataset conforms to PDS Standards Version 3.6 and includes experiment documentation.
NASA provides an updated compilation of asteroid families and clusters. The data results from applying the Hierarchical Clustering Method to proper elements for approximately 120,000 asteroids. It was last updated in March 2026 and includes Bus taxonomy classifications from spectroscopic surveys where available.
OSIRIS Narrow Angle Camera images were acquired during the PRELANDING phase of the Rosetta mission at comet 67P/Churyumov–Gerasimenko. The data covers the period from 2014-07-02T08:35:00.000 to 2014-08-01T09:59:59.000 and is version V2.0, which supersedes previous deliveries. The dataset originates from the National Aeronautics and Space Administration.
From 16th September 2007 to 22nd January 2008, this dataset contains raw navigation camera (NAVCAM) images from the ESA Rosetta spacecraft's second Earth swing-by during its cruise to comet 67P/Churyumov-Gerasimenko. The data was produced by the National Aeronautics and Space Administration and represents version 1.1, which supersedes an earlier release with updated browse images and FITS file additions.
Percent Polarized data from the STEREO SECCHI Cor2 telescopes, capturing images of the Sun's corona and heliosphere. The data is provided at a 1-hour cadence and full 2048x2048 pixel resolution, generally available within about three days of observation. This dataset is produced by the National Aeronautics and Space Administration (NASA).
Data from the Prelanding phase of the Rosetta mission to comet 67P/Churyumov–Gerasimenko, collected between 2014-03-29 and 2014-11-18. It contains level 3 science data acquired by the DFMS and RTOF sensors of the ROSINA instrument. The dataset is provided by the National Aeronautics and Space Administration and was last updated in March 2026.
STEREO SECCHI Cor2 telescopes provide percent polarized data of the Sun's corona at a cadence of approximately one hour. The images are full resolution at 2048 by 2048 pixels and are generally available within about three days of observation. The data is produced by the National Aeronautics and Space Administration.
OSIRIS Narrow Angle Camera images were acquired during the PRELANDING phase of the Rosetta mission at comet 67P/Churyumov–Gerasimenko. The data covers the period from 2014-08-01 to 2014-09-02 and is version V2.0, which supersedes previous deliveries. The dataset is provided by the National Aeronautics and Space Administration.
Mass spectrometry science data from the Rosetta mission's ROSINA instrument, specifically the DFMS and RTOF sensors. The data was collected between 2016-06-28 and 2016-06-30 during the Extension phase 3 of the mission to comet 67P/Churyumov–Gerasimenko. Version 2.0 of this dataset features an enhanced mass scale for selected masses and improved offset removal, with corrupted files removed.
Arecibo Observatory radar images of the Moon's surface at a 12.6 cm wavelength. The National Aeronautics and Space Administration produced these scaled backscatter cross-section images, which are projected onto a Mercator grid with 0.01-degree longitude spacing per pixel. The data are corrected for antenna beam shape but not for scattering variations with incidence angle.
NASA's ROSETTA-ORBITER 67P OSIWAC 5 EXT1-MTP025 DDR-GEO V1.0 dataset contains pixel-precise georeferencing information derived from images of comet 67P/Churyumov-Gerasimenko. The data was acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the ROSETTA EXTENSION 1 mission phase from January to February 2016. This V1.0 version is the first release, corrected after an October 2018 external peer review.
Calibrated data from the MUPUS instrument onboard the ROSETTA Lander, acquired during the SDL phase. The primary target is comet 67P/Churyumov-Gerasimenko. The data conform to Planetary Data System Standards Version 3.6.
144-second averaged data files from the URAP radio astronomy instrument. The dataset likely contains averaged electric field measurements. It is produced by the National Aeronautics and Space Administration.
NASA's RAR 144 second averaged data files contain averaged electric field measurements from radio astronomy observations. The dataset is described in a user's guide document detailing its contents and format. The data was last updated on March 13, 2026.