INTERPLANETARY DUST PARTICLES AS SAMPLES OF ICY ASTEROIDS
Meteorites have long been considered as reflections of the compositional diversity of main belt asteroids and consequently they have been used to decipher their origin, formation, and evolution. However, while some meteorites are known to sample the surfaces of metallic, rocky and hydrated asteroids...
Main Authors: | Vernazza, P., Marsset, M., Beck, P., Birlan, M., Brunetto, R., Djouadi, Z., Dumas, C., Merouane, S., Mousis, O., Zanda, B., Binzel, Richard P, DeMeo, Francesca E |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2015
|
Online Access: | http://hdl.handle.net/1721.1/98365 |
Similar Items
-
Active Asteroid (6478) Gault: A Blue Q-type Surface below the Dust?
by: Marsset, Michaël, et al.
Published: (2021) -
Similar origin for low- and high-albedo Jovian Trojans and Hilda asteroids?
by: Marsset, M., et al.
Published: (2015) -
Rotationally resolved spectroscopy of asteroid pairs: No spectral variation suggests fission is followed by settling of dust
by: Polishook, David, et al.
Published: (2017) -
Compositional characterisation of the Themis family
by: Marsset, M., et al.
Published: (2017) -
COMPOSITIONAL HOMOGENEITY OF CM PARENT BODIES
by: Vernazza, P., et al.
Published: (2021)