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}
},
{
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},
{
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},
{
"orgName": "Goddard Institute for Space Studies (GISS)",
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},
{
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},
{
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},
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},
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}
},
{
"orgName": "Ocean Ecology Laboratory",
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},
{
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}
},
{
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}
},
{
"orgName": "Terrestrial Information Systems Laboratory",
"orgShortName": "Terrestrial Information Systems",
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}
},
{
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},
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},
{
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},
{
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{
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},
{
"orgName": "Astroparticle Physics Laboratory",
"orgShortName": "Astroparticle Physics Laboratory",
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"secondary": "astroparticles"
}
},
{
"orgName": "X-ray Astrophysics Laboratory",
"orgShortName": "X-ray Astrophysics Laboratory",
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}
},
{
"orgName": "Gravitational Astrophysics Laboratory",
"orgShortName": "Gravitational Astrophysics Laboratory",
"orgCode": "663",
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"router": {
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"secondary": "gravity"
}
},
{
"orgName": "Observational Cosmology Laboratory",
"orgShortName": "Observational Cosmology Laboratory",
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"router": {
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}
},
{
"orgName": "Exoplanets and Stellar Astrophysics Laboratory",
"orgShortName": "Exoplanets and Stellar Astrophysics Laboratory",
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},
{
"orgName": "Heliophysics Science Division",
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}
},
{
"orgName": "Solar Physics Laboratory",
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}
},
{
"orgName": "Heliospheric Physics Laboratory ",
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"secondary": "heliospheric"
}
},
{
"orgName": "Geospace Physics Laboratory",
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"secondary": "geospace"
}
},
{
"orgName": "Space Weather Laboratory",
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"secondary": "spaceweather"
}
},
{
"orgName": "Ionospheric, Thermospheric, Mesospheric (ITM) Physics Laboratory",
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"secondary": "itmphysics"
}
},
{
"orgName": "Solar System Exploration Division",
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"secondary": null
}
},
{
"orgName": "Solar System Exploration Data Services Office",
"orgShortName": "Solar System Exploration Data Services Office",
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"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "dataarchives"
}
},
{
"orgName": "Astrochemistry Laboratory",
"orgShortName": "Astrochemistry Laboratory",
"orgCode": "691",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "astrochemistry"
}
},
{
"orgName": "Planetary Systems Lab",
"orgShortName": "Planetary Systems Laboratory",
"orgCode": "693",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "planetarysystems"
}
},
{
"orgName": "Planetary Magnetospheres Lab",
"orgShortName": "Planetary Magnetospheres Laboratory",
"orgCode": "695",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "magnetospheres"
}
},
{
"orgName": "Planetary Geology, Geophysics & Geochemistry Lab",
"orgShortName": "Planetary Geology, Geophysics & Geochemistry Lab",
"orgCode": "698",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "p3g"
}
},
{
"orgName": "Planetary Environments Laboratory ",
"orgShortName": "Planetary Environments Laboratory",
"orgCode": "699",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "atmosenvironments"
}
}
]
Comet Interceptor (CI)
The Comet Interceptor mission is an ESA led mission with 3 spacecraft elements working together to perform the first close encounter to a long period comet. One spacecraft will make remote and in situ observations of the comet from afar, while two other spacecraft will be deployed to venture closer to the target, carrying complementary instrument payloads, to build up a 3D picture of the comet. NASA Goddard is supporting the development of the Multispectral InfraRed Molecular and Ices Sensor (MIRMIS) onboard this mission. The instrument is composed of three channels (NIR is a 0.9 to 1.7 µm hyperspectral imager, MIR is a 2.5 to 5 µm point spectrometers and the Thermal Infrared Imager TIRI is a 6 to 25 µm multispectral thermal mapper. These sensors target diagnostic spectral features of water, carbon dioxide, water ice, organics and several minerals and these measurements are critical to establish the thermophysical properties of the comet.
The Comet Interceptor mission is an ESA led mission with 3 spacecraft elements working together to perform the first close encounter to a long period comet. One spacecraft will make remote and in situ observations of the comet from afar, while two other spacecraft will be deployed to venture closer to the target, carrying complementary instrument payloads, to build up a 3D picture of the comet. NASA Goddard is supporting the development of the Multispectral InfraRed Molecular and Ices Sensor (MIRMIS) onboard this mission. The instrument is composed of three channels (NIR is a 0.9 to 1.7 µm hyperspectral imager, MIR is a 2.5 to 5 µm point spectrometers and the Thermal Infrared Imager TIRI is a 6 to 25 µm multispectral thermal mapper. These sensors target diagnostic spectral features of water, carbon dioxide, water ice, organics and several minerals and these measurements are critical to establish the thermophysical properties of the comet.
Related Publications
2024. "Modelling for Comet Interceptor's Modular InfraRed Molecules and Ices Sensor.", LPI Contributions, 3040 1386 [Proceedings]
2024. "The Comet Interceptor Mission.", Space Science Reviews, 220 (1): 9 [10.1007/s11214-023-01035-0] [Journal Article/Letter]