Outer Main Belt asteroids: Identification and distribution of four 3-μm spectral groups

By D. Takir, J. Emery. 2011

180 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Ecology

View Paper: https://www.semanticscholar.org/paper/c0c4158407e0749cb9880a75fc9896ff3b6f7f28

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. F. DeMeo
2. Kevin J. Walsh
3. C. Alexander
4. Clark R. Chapman
5. Stefano Mottola
6. C. Lantz
7. Jean-Loup Bertaux
8. G. Kovacs

In Ecology

1. F. DeMeo
2. Kevin J. Walsh
3. C. Alexander
4. Clark R. Chapman
5. R. Binzel
6. Benoît Carry
7. S. Bus
8. T. Burbine

Citations in the corpus

• The Compositional Structure of the Asteroid Belt (2015, background): “Asteroid spectra at these wavelengths are categorized by the presence of and shape of a 3-micron absorption feature indicating hydrated minerals or phyllosilicates (Takir & Emery 2012, Rivkin et al., this volume).”
• The primordial nucleus of comet 67P/Churyumov-Gerasimenko (2015, background): “Takir & Emery (2012) measured the 0.8–2.5 µm and 1.9– 4.1 µm spectra of 28 outer main belt asteroids.”
• Ion irradiation of carbonaceous chondrites: A new view of space weathering on primitive asteroids (2017, background): “The 2.7 µm band lies within the wavelength range of strong absorption by water vapor in Earth atmosphere [e.g. Takir & Emery, 2012], 17 AC CE PT ED M AN US CR IP T thus it will be impossible to use this spectroscopic information of SpWe from remote sensing observations.”