Dust from the outer Solar System comes down to Earth
Author:
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
https://www.nature.com/articles/s41550-022-01662-7.pdf
Reference5 articles.
1. Nesvorný, D. et al. Cometary origin of the zodiacal cloud and carbonaceous micrometeorites. Implications for hot debris disks. Astrophys. J. 713, 816–836 (2010). This paper proposes a dust model for the origin of the zodiacal cloud.
2. Poppe, A. R. An improved model for interplanetary dust fluxes in the outer Solar System. Icarus. 264, 369–386 (2016). This paper describes the dust mass and dust production in the Kuiper belt.
3. Bradley, J. P., Brownlee, D. E. & Fraundorf, P. Discovery of nuclear tracks in interplanetary dust. Science 226, 1432–1434 (1984). This paper reports the detection of tracks in IDPs using TEM methods.
4. Christoffersen, R. & Buseck, P. R. Mineralogy of interplanetary dust particles from the ‘olivine’ infrared class. Earth Planet. Sci. Lett. 78, 53–66 (1986). This paper is a systematic study of olivine-rich IDPs and their space exposure ages.
5. Keller, L. P., Berger, E. L., Zhang, S. & Christoffersen, R. Solar energetic particle tracks in lunar samples: A transmission electron microscope calibration and implications for lunar space weathering. Met. Planet. Sci. 56, 1685–1707 (2021). This paper reports the track production rate calibration used to determine IDP exposure ages.
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