Endre søk
RefereraExporteraLink to record
Permanent link

Direct link
Referera
Referensformat
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Annet format
Fler format
Språk
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Annet språk
Fler språk
Utmatningsformat
  • html
  • text
  • asciidoc
  • rtf
Infrared Spectrometer for ExoMars: A Mast-Mounted Instrument for the Rover
Space Research Institute IKI, Moscow.
Space Research Institute IKI, Moscow.
Space Research Institute IKI, Moscow.
Space Research Institute IKI, Moscow.
Vise andre og tillknytning
2017 (engelsk)Inngår i: Astrobiology, ISSN 1531-1074, E-ISSN 1557-8070, Vol. 17, nr 6-7, s. 542-564Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

ISEM (Infrared Spectrometer for ExoMars) is a pencil-beam infrared spectrometer that will measure reflected solar radiation in the near infrared range for context assessment of the surface mineralogy in the vicinity of the ExoMars rover. The instrument will be accommodated on the mast of the rover and will be operated together with the panoramic camera (PanCam), high-resolution camera (HRC). ISEM will study the mineralogical and petrographic composition of the martian surface in the vicinity of the rover, and in combination with the other remote sensing instruments, it will aid in the selection of potential targets for close-up investigations and drilling sites. Of particular scientific interest are water-bearing minerals, such as phyllosilicates, sulfates, carbonates, and minerals indicative of astrobiological potential, such as borates, nitrates, and ammonium-bearing minerals. The instrument has an ∼1° field of view and covers the spectral range between 1.15 and 3.30 μm with a spectral resolution varying from 3.3 nm at 1.15 μm to 28 nm at 3.30 μm. The ISEM optical head is mounted on the mast, and its electronics box is located inside the rover's body. The spectrometer uses an acousto-optic tunable filter and a Peltier-cooled InAs detector. The mass of ISEM is 1.74 kg, including the electronics and harness. The science objectives of the experiment, the instrument design, and operational scenarios are described.

sted, utgiver, år, opplag, sider
Mary Ann Liebert, 2017. Vol. 17, nr 6-7, s. 542-564
HSV kategori
Forskningsprogram
Atmosfärsvetenskap
Identifikatorer
URN: urn:nbn:se:ltu:diva-65102DOI: 10.1089/ast.2016.1543ISI: 000406038400003PubMedID: 28731817Scopus ID: 2-s2.0-85025436062OAI: oai:DiVA.org:ltu-65102DiVA, id: diva2:1133318
Merknad

Validerad; 2017; Nivå 2; 2017-08-16 (andbra)

Tilgjengelig fra: 2017-08-15 Laget: 2017-08-15 Sist oppdatert: 2019-05-14bibliografisk kontrollert

Open Access i DiVA

Fulltekst mangler i DiVA

Andre lenker

Forlagets fulltekstPubMedScopus

Personposter BETA

Martin-Torres, JavierZorzano Mier, Maria-Paz

Søk i DiVA

Av forfatter/redaktør
Martin-Torres, JavierZorzano Mier, Maria-Paz
Av organisasjonen
I samme tidsskrift
Astrobiology

Søk utenfor DiVA

GoogleGoogle Scholar

doi
pubmed
urn-nbn

Altmetric

doi
pubmed
urn-nbn
Totalt: 35 treff
RefereraExporteraLink to record
Permanent link

Direct link
Referera
Referensformat
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Annet format
Fler format
Språk
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Annet språk
Fler språk
Utmatningsformat
  • html
  • text
  • asciidoc
  • rtf