Predictions for the detection of Earth and Mars Trojan asteroids by the Gaia satellite

The European Space Agency Gaia satellite, planned for launch in late 2013, will perform systematic astrometric observations of the whole sky over a five year period. During this mission many thousands of Solar System Objects down to magnitude V =20 will be observed including Near-Earth Asteroids and...

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Main Authors: Todd, M., Tanga, P., Coward, D., Zadnik, Marjan
Format: Journal Article
Published: Oxford University Press 2014
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/30744
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author Todd, M.
Tanga, P.
Coward, D.
Zadnik, Marjan
author_facet Todd, M.
Tanga, P.
Coward, D.
Zadnik, Marjan
author_sort Todd, M.
building Curtin Institutional Repository
collection Online Access
description The European Space Agency Gaia satellite, planned for launch in late 2013, will perform systematic astrometric observations of the whole sky over a five year period. During this mission many thousands of Solar System Objects down to magnitude V =20 will be observed including Near-Earth Asteroids and objects at Solar elongations a slow as 45 °, which are difficult to observe with ground-based telescopes. We simulated the detection of Trojan asteroids in the orbits of Earth and Mars by Gaia. We find that Gaia will not detect the Earth Trojan 2010 TK7 although it will detect any Earth Trojans with diameters larger than 600 m. We also find that Gaia will detect the currently known Mars Trojans and could discover more than 100 new Mars Trojans as small as 400 m in diameter. The results of the Gaia mission will test the predictions about the Mars Trojan asteroid population and lead to greater understanding about the evolution of the Solar System.
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spelling curtin-20.500.11937-307442017-09-13T15:10:07Z Predictions for the detection of Earth and Mars Trojan asteroids by the Gaia satellite Todd, M. Tanga, P. Coward, D. Zadnik, Marjan asteroids: general – planets and satellites: general – celestial mechanics methods: numerical – methods: observational – methods: statistical – - minor planets The European Space Agency Gaia satellite, planned for launch in late 2013, will perform systematic astrometric observations of the whole sky over a five year period. During this mission many thousands of Solar System Objects down to magnitude V =20 will be observed including Near-Earth Asteroids and objects at Solar elongations a slow as 45 °, which are difficult to observe with ground-based telescopes. We simulated the detection of Trojan asteroids in the orbits of Earth and Mars by Gaia. We find that Gaia will not detect the Earth Trojan 2010 TK7 although it will detect any Earth Trojans with diameters larger than 600 m. We also find that Gaia will detect the currently known Mars Trojans and could discover more than 100 new Mars Trojans as small as 400 m in diameter. The results of the Gaia mission will test the predictions about the Mars Trojan asteroid population and lead to greater understanding about the evolution of the Solar System. 2014 Journal Article http://hdl.handle.net/20.500.11937/30744 10.1093/mnras/stt2223 Oxford University Press fulltext
spellingShingle asteroids: general – planets and satellites: general – celestial mechanics
methods: numerical – methods: observational – methods: statistical – - minor planets
Todd, M.
Tanga, P.
Coward, D.
Zadnik, Marjan
Predictions for the detection of Earth and Mars Trojan asteroids by the Gaia satellite
title Predictions for the detection of Earth and Mars Trojan asteroids by the Gaia satellite
title_full Predictions for the detection of Earth and Mars Trojan asteroids by the Gaia satellite
title_fullStr Predictions for the detection of Earth and Mars Trojan asteroids by the Gaia satellite
title_full_unstemmed Predictions for the detection of Earth and Mars Trojan asteroids by the Gaia satellite
title_short Predictions for the detection of Earth and Mars Trojan asteroids by the Gaia satellite
title_sort predictions for the detection of earth and mars trojan asteroids by the gaia satellite
topic asteroids: general – planets and satellites: general – celestial mechanics
methods: numerical – methods: observational – methods: statistical – - minor planets
url http://hdl.handle.net/20.500.11937/30744