API using comprehensive data set from The Meteoritical Society that contains information on all of the known meteorite landings.

This data set contains meteoroid orbits from photographic, TV system, and radar meteoroid surveys collected from the International Astronomical Union Meteor Data Center (IAU MDC) by Duncan Steel and reviewed and discussed in Steel (1996). The data cover the time period 1940-1983.

This data set contains meteoroid orbits from photographic, TV system, and radar meteoroid surveys collected from the International Astronomical Union Meteor Data Center (IAU MDC) by Duncan Steel and reviewed and discussed in Steel (1996). The data cover the time period 1940-1983.

Image database of meteorites of martian origin collected by the Antarctic Search for Meteorites Program.

Current models do not sufficiently explain target rock-projectile mixing and ejecta blanket formation for small impact craters (i.e., <2km diameter). For example, due to the size of Meteor Crater and the low-velocity at which materials were excavated from the transient crater, the extent of target rock-projectile mixing is expected to be minor. However, based on drilling notes from Dr. David Roddy and preliminary work done at the USGS, we found lithologic mixing is much more prevalent throughout the ejecta blanket. We have used the USGS Meteor Crater sample collection to investigate the internal stratigraphy and spatial distribution of impact-generated materials in the ejecta blanket to better understand cratering processes involving votatile-rich sedimentary target rocks. Data presented here are the measurements and summarized results from our lithostratigraphic analysis of the continuous ejecta blanket at Meteor Crater. 'Lithostratigraphic_analysis_measurements' file includes all of our mass and volume measurements for each sample, and 'Lithostratigraphic_analysis_summary' file is our summarized results, which includes an assigned unit for each sample based on the contrasting mixtures of target rocks (from our measurements), and the overall thickness of each identified unit across the selected transects. These data are the supplementary materials associated with a manuscript that will soon be published in a peer-review journal.

The Meteor-3 Total Ozone Mapping Spectrometer (TOMS) version 8 daily ground station overpass data product contains total column ozone, UV aerosol index, Lambertian effective surface reflectivity (Rayleigh corrected), UV aerosol index and sulfur dioxide index values. The overpass data files contain the data derived from the best-matched TOMS field-of-view (FOV) to a site for every day the TOMS instrument was operational. The data are stored in an ASCII format.TOMS data were produced by the Laboratory for Atmospheres at NASA Goddard Space Flight Center (Code 614).

A Level 2 data file containing all the species products for a single lunar event

This data set includes spectra of meteorite samples reported by M. J. Gaffey in the 1976 paper 'Spectral reflectance characteristics of the meteorite classes' (JGR 81, 905) [GAFFEY1976].

Collected shape and gravity models and related data for the NEAR targets 433 Eros and 253 Mathilde.