In search of the source of asteroid (101955) Bennu: Applications of the stochastic YORP model

By William Bottke, David Vokrouhlický, Kevin J. Walsh, M. Delbo’, Patrick Michel, Dante S. Lauretta, H. Campins, H. Connolly, Daniel J. Scheeres, Steven R. Chelsey. 2015

154 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/1c352e3f3d20fde318377e83e82a76cd6827d4b2

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In Astronomy and Astrophysics

1. Kevin J. Walsh
2. William Bottke
3. V. Hamilton
4. R. Binzel
5. Dante S. Lauretta
6. Daniel J. Scheeres
7. H. Connolly
8. Jason P. Dworkin

Citations in the corpus

• OSIRIS-REx: Sample Return from Asteroid (101955) Bennu (2017, background): “The fragment that became Bennu was eventually delivered to near-Earth space via a combination of Yarkovsky-induced drift and interaction with giant-planet gravitational resonances (Campins et al. 2010; Bottke et al. 2015).”
• Asteroid family ages (2015, unknown): “, 2006b) give an age of 280± 112 My, which is higher but consistent; (Bottke et al., 2015) by a different method give an age 170 −30, which is lower but consistent with the IN side.”
• OCAMS: The OSIRIS-REx Camera Suite (2017, background): “Researchers believe Bennu, a B-type asteroid and possible CM-chondrite spectral analog, to be primitive and volatile-rich (Clark et al. 2011), and possibly derived from the inner regions of the main belt (Campins et al. 2010; Bottke et al. 2015).”