The Stardust Mission: Analyzing Samples from the Edge of the Solar System
By D. Brownlee. 2014
182 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/6a87284d91e1382ae8d64fb7cd440bc7d2005f49
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In Astronomy and Astrophysics
- D. Whittet
- P. Gerakines
- A. Boogert
- F. Ciesla
- Yves Langevin
- Dante S. Lauretta
- Edward B. Bierhaus
- L. Nittler
Citations in the corpus
- Melting and differentiation of early-formed asteroids: The perspective from high precision oxygen isotope studies (2017, unknown): “Solid particles collected from the Jupiter family comet 81P/Wild 2 by the NASA Stardust mission included chondrules and refractory inclusions that were most likely formed close to the early Sun and then subsequently transported to the cold outer regions of the Solar System (Brownlee, 2014).”
- The OSIRIS-REx Spacecraft and the Touch-and-Go Sample Acquisition Mechanism (TAGSAM) (2018, background): “4) is nearly identical to the SRC for the Stardust mission, a successful NASA mission that captured samples from comet Wild 2 and returned them to the Earth in 2006 (Brownlee 2014).”
- Carbon-rich dust in comet 67P/Churyumov-Gerasimenko measured by COSIMA/Rosetta (2017, methodology): “However, a quantification of the carbonaceous materials in the particles of 81P/Wild 2 was not possible due to the high impact speed and collection method of these particles (Sandford et al. 2010; Brownlee 2014).”
- Observations of the Icy Universe (2015, background): “The Stardust mission revealed that refractory dust may have formed close to the early Sun, moving radially outward, accumulating ices along the way and thus diluting any presolar components in the outer, comet formation zones (Brownlee, 2014).”
- Astrophysics with Extraterrestrial Materials (2016, background): “Evidence for mixing is found in a variety of forms, but the samples the Stardust mission returned from the Jupiter-family (Kuiper Belt) comet Wild-2 have motivated most discussions in recent years (Figure 2) (Brownlee et al. 2006, Brownlee 2014).”