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Data · dataset · 2025

FORNASIER SPECTRA OF M ASTEROIDS

Listed in Open NASA

This data set contains reduced composite visual and near-infrared spectra of thirty M-type asteroids, observed over the years 2004-2008 and presented in Fornasier et al. (2010).

Description

The spectra were taken with the Dolores and NICS instruments at the Telescopio Nationale Galileo (TNG) in La Palma, with the EMMI and SOFI instruments at the ESO New Technology Telescope (NTT) in Chile, and with the SPeX instrument at the Infrared Telescope Facility (IRTF) in Hawaii.

The individual spectra from the various instruments used to produce the composite spectra are also included.

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Provenance · 1 source records, 7 field assertions
SourceKeyLast seenRaw
Open NASA8d28eacf-b1f1-48bd-828e-aeb17773e51317 h agoJSON v1
FieldAssertionExtractorEvidence
concepts[field].local:field:ocean-atmosphericmapping · open nasa govconnector:open_nasa_gov@1.0.0
created_datesource · open nasa govconnector:open_nasa_gov@1.0.0
descriptionsource · open nasa govconnector:open_nasa_gov@1.0.0/notes
license_textsource · open nasa govconnector:open_nasa_gov@1.0.0
publication_datesource · open nasa govconnector:open_nasa_gov@1.0.0
titlesource · open nasa govconnector:open_nasa_gov@1.0.0/title
updated_datesource · open nasa govconnector:open_nasa_gov@1.0.0