Volume 608, December 2017
|Number of page(s)||8|
|Section||Planets and planetary systems|
|Published online||08 December 2017|
Composition of Jupiter irregular satellites sheds light on their origin
1 Space Physics Laboratory, Vikram Sarabhai Space Centre, Thiruvananthapuram, 695022 Kerala, India
2 Lunar and Planetary Laboratory, University of Arizona, 1629 E University Blvd, Tucson, AZ 85721-0092, USA
3 Deutsches SOFIA Institut, Universität Stuttgart, Pfaffenwaldring 29, 70569 Stuttgart, Germany
4 SOFIA Science Center, NASA Ames Research Center, Mail Stop N211-1, Mo ett Field, CA 94035, USA
5 Department of Geography, University of Winnipeg, 515 Portage Avenue, Winnipeg, Manitoba R3B 2E9, Canada
6 Physical Research Laboratory, Ahmedabad, 380009 Gujarat, India
7 Planetary Science Institute, 1700 East Fort Lowell Road, Tucson, AZ 85719, USA
Received: 26 December 2016
Accepted: 10 September 2017
Context. Irregular satellites of Jupiter with their highly eccentric, inclined and distant orbits suggest that their capture took place after the giant planet migration.
Aims. We aim to improve our understanding of the surface composition of irregular satellites of Jupiter to gain insight into a narrow time window when our solar system was forming.
Methods. We observed three Jovian irregular satellites, Himalia (JVI), Elara (JVII), and Carme (JXI), using a medium-resolution 0.8–5.5 μm spectrograph, SpeX on the NASA Infrared Telescope Facility (IRTF). Using a linear spectral unmixing model we have constrained the major mineral phases on the surface of these three bodies.
Results. Our results confirm that the surface of Himalia (JVI), Elara (JVII), and Carme (JXI) are dominated by opaque materials such as those seen in carbonaceous chondrite meteorites. Our spectral modeling of NIR spectra of Himalia and Elara confirm that their surface composition is the same and magnetite is the dominant mineral. A comparison of the spectral shape of Himalia with the two large main C-type asteroids, Themis (D ~ 176 km) and Europa (D ~ 352 km), suggests surface composition similar to Europa. The NIR spectrum of Carme exhibits blue slope up to 1.5 μm and is spectrally distinct from those of Himalia and Elara. Our model suggests that it is compositionally similar to amorphous carbon.
Conclusions. Himalia and Elara are compositionally similar but differ significantly from Carme. These results support the hypotheses that the Jupiter’s irregular satellites are captured bodies that were subject to further breakup events and clustered as families based on their similar physical and surface compositions.
Key words: planets and satellites: individual: Himalia / planets and satellites: surfaces / techniques: spectroscopic / planets and satellites: individual: Elara / planets and satellites: individual: Carme
© ESO, 2017
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