Infrared Spectrometer for ExoMars: A Mast-Mounted Instrument for the Rover

O. I. Korablev; Y. Dobrolensky; N. Evdokimova; A. A. Fedorova; V. O. Kuzmin; S. N. Mansevich; E. A. Cloutis; John Carter; F. Poulet; J. Flahaut; A. Griffiths; Matthew Gunn; N. Schmitz; J. Martín-Torres; M. -P. Zorzano; D. S. Rodionov; J. L. Vago; A. V. Stepanov; A. Y. Titanov; N. A. Vyazovetsky; A. Y. Trokhimovskiy; A. G. Sapgir; Y. K. Kalinnikov; Y. S. Ivanov; A. A. Shapkin; A. Y. Ivanov

doi:10.1089/ast.2016.1543

Infrared Spectrometer for ExoMars: A Mast-Mounted Instrument for the Rover

O. I. Korablev, Y. Dobrolensky, N. Evdokimova, A. A. Fedorova, V. O. Kuzmin, S. N. Mansevich, E. A. Cloutis, John Carter, F. Poulet, J. Flahaut, A. Griffiths, Matthew Gunn, N. Schmitz, J. Martín-Torres, M. -P. Zorzano, D. S. Rodionov, J. L. Vago, A. V. Stepanov, A. Y. Titanov, N. A. VyazovetskyA. Y. Trokhimovskiy, A. G. Sapgir, Y. K. Kalinnikov, Y. S. Ivanov, A. A. Shapkin, A. Y. Ivanov

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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 ammoniumbearing minerals. The instrument has an *1 field of view and covers the spectral range between 1.15 and 3.30 mm with a spectral resolution varying from 3.3 nm at 1.15 mm to 28 nm at 3.30 mm. 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.

Iaith wreiddiol	Saesneg
Tudalennau (o-i)	542-564
Nifer y tudalennau	23
Cyfnodolyn	Astrobiology
Cyfrol	17
Rhif cyhoeddi	6-7
Dynodwyr Gwrthrych Digidol (DOIs)	https://doi.org/10.1089/ast.2016.1543
Statws	Cyhoeddwyd - 01 Gorff 2017

Mynediad at Ddogfen

10.1089/ast.2016.1543Trwydded: Aneglur 2

Infrared Spectrometer for ExoMars (ISEM), a Mast-Mounted Instrument for the RoverLlawysgrif awdur wedi’i dderbyn, 1.94 MB

Cysylltiad parhaol

Dolen barhaus

Matt Gunn
- mmgaber.acuk
- Adran Ffiseg - Senior Research Fellow
Unigolyn: Ymchwil

2 Wedi Gorffen

Stereo wide-angle cameras for the Exomars Panoramic Camera Instrument - Part D
Gunn, M. (Prif Ymchwilydd)
European Space Agency
01 Awst 2015 → 31 Rhag 2015
Prosiect: Ymchwil a ariannwyd yn allanol
Stereo wide angle cameras for the Exomars Panoramic camera instrument, PART C
Barnes, D. (Prif Ymchwilydd)
Science & Technology Facilities Council
01 Ebr 2013 → 31 Maw 2016
Prosiect: Ymchwil a ariannwyd yn allanol

Dyfynnu hyn

Korablev, O. I., Dobrolensky, Y., Evdokimova, N., Fedorova, A. A., Kuzmin, V. O., Mansevich, S. N., Cloutis, E. A., Carter, J., Poulet, F., Flahaut, J., Griffiths, A., Gunn, M., Schmitz, N., Martín-Torres, J., Zorzano, M. .-P., Rodionov, D. S., Vago, J. L., Stepanov, A. V., Titanov, A. Y., ... Ivanov, A. Y. (2017). Infrared Spectrometer for ExoMars: A Mast-Mounted Instrument for the Rover. Astrobiology, 17(6-7), 542-564. https://doi.org/10.1089/ast.2016.1543

@article{9e3fd859c40242b482da15f778818fc6,

title = "Infrared Spectrometer for ExoMars: A Mast-Mounted Instrument for the Rover",

abstract = "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 ammoniumbearing minerals. The instrument has an *1 field of view and covers the spectral range between 1.15 and 3.30 mm with a spectral resolution varying from 3.3 nm at 1.15 mm to 28 nm at 3.30 mm. The ISEM optical head is mounted on the mast, and its electronics box is located inside the rover{\textquoteright}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.",

author = "Korablev, {O. I.} and Y. Dobrolensky and N. Evdokimova and Fedorova, {A. A.} and Kuzmin, {V. O.} and Mansevich, {S. N.} and Cloutis, {E. A.} and John Carter and F. Poulet and J. Flahaut and A. Griffiths and Matthew Gunn and N. Schmitz and J. Mart{\'i}n-Torres and Zorzano, {M. -P.} and Rodionov, {D. S.} and Vago, {J. L.} and Stepanov, {A. V.} and Titanov, {A. Y.} and Vyazovetsky, {N. A.} and Trokhimovskiy, {A. Y.} and Sapgir, {A. G.} and Kalinnikov, {Y. K.} and Ivanov, {Y. S.} and Shapkin, {A. A.} and Ivanov, {A. Y.}",

year = "2017",

month = jul,

day = "1",

doi = "10.1089/ast.2016.1543",

language = "English",

volume = "17",

pages = "542--564",

journal = "Astrobiology",

issn = "1531-1074",

publisher = "Mary Ann Liebert Inc.",

number = "6-7",

}

Korablev, OI, Dobrolensky, Y, Evdokimova, N, Fedorova, AA, Kuzmin, VO, Mansevich, SN, Cloutis, EA, Carter, J, Poulet, F, Flahaut, J, Griffiths, A, Gunn, M, Schmitz, N, Martín-Torres, J, Zorzano, M-P, Rodionov, DS, Vago, JL, Stepanov, AV, Titanov, AY, Vyazovetsky, NA, Trokhimovskiy, AY, Sapgir, AG, Kalinnikov, YK, Ivanov, YS, Shapkin, AA & Ivanov, AY 2017, 'Infrared Spectrometer for ExoMars: A Mast-Mounted Instrument for the Rover', Astrobiology, cyfrol. 17, rhif 6-7, tt. 542-564. https://doi.org/10.1089/ast.2016.1543

TY - JOUR

T1 - Infrared Spectrometer for ExoMars

T2 - A Mast-Mounted Instrument for the Rover

AU - Korablev, O. I.

AU - Dobrolensky, Y.

AU - Evdokimova, N.

AU - Fedorova, A. A.

AU - Kuzmin, V. O.

AU - Mansevich, S. N.

AU - Cloutis, E. A.

AU - Carter, John

AU - Poulet, F.

AU - Flahaut, J.

AU - Griffiths, A.

AU - Gunn, Matthew

AU - Schmitz, N.

AU - Martín-Torres, J.

AU - Zorzano, M. -P.

AU - Rodionov, D. S.

AU - Vago, J. L.

AU - Stepanov, A. V.

AU - Titanov, A. Y.

AU - Vyazovetsky, N. A.

AU - Trokhimovskiy, A. Y.

AU - Sapgir, A. G.

AU - Kalinnikov, Y. K.

AU - Ivanov, Y. S.

AU - Shapkin, A. A.

AU - Ivanov, A. Y.

PY - 2017/7/1

Y1 - 2017/7/1

N2 - 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 ammoniumbearing minerals. The instrument has an *1 field of view and covers the spectral range between 1.15 and 3.30 mm with a spectral resolution varying from 3.3 nm at 1.15 mm to 28 nm at 3.30 mm. 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.

AB - 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 ammoniumbearing minerals. The instrument has an *1 field of view and covers the spectral range between 1.15 and 3.30 mm with a spectral resolution varying from 3.3 nm at 1.15 mm to 28 nm at 3.30 mm. 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.

U2 - 10.1089/ast.2016.1543

DO - 10.1089/ast.2016.1543

M3 - Article

C2 - 28731817

SN - 1531-1074

VL - 17

SP - 542

EP - 564

JO - Astrobiology

JF - Astrobiology

IS - 6-7

ER -

Infrared Spectrometer for ExoMars: A Mast-Mounted Instrument for the Rover

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Stereo wide-angle cameras for the Exomars Panoramic Camera Instrument - Part D

Stereo wide angle cameras for the Exomars Panoramic camera instrument, PART C

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