Results 11 to 20 of about 10,634 (253)
Time/Frequency Analysis of Terrestrial Impack Crater Records [PDF]
Journal of Astronomy and Space Sciences, 2006 The terrestrial impact cratering record recently has been examined in the time domain by Chang & Moon (2005). It was found that the ˜ 26 Myr periodicity in the impact cratering rate exists over the last ˜ 250 Myrs.
Heon-Young Chang
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Universe, 2022 Presolar grains are microscopic dust grains that formed in the stellar winds or explosions of ancient stars that died before the formation of the solar system.
Nan Liu, Sergio Cristallo, Diego Vescovi
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Atmosphere, 2023 Advancements in space exploration and sample return technology present a unique opportunity to leverage sample return capsules (SRCs) towards studying atmospheric entry of meteoroids and asteroids.
Elizabeth A. Silber +2 more
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Asteroid–Meteoroid Complexes [PDF]
, 2019 Chapter 8 in the book "Meteoroids: Sources of Meteors on Earth and Beyond", Cambridge University Press ...
Kasuga, Toshihiro, Jewitt, David
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Atmosphere, 2018 Nitric oxide (NO) is a critical indicator of energy deposition in the lower thermosphere because of its formational pathways. Thus, it is important to constrain sources of NO, such as meteoroid generated hypersonic flows below 95 km altitude.
Elizabeth A. Silber +3 more
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SPACE DENSITY DISTRIBUTION OF METEOROIDS OVER THE SPHERE WITH RADIUS 1 A.U.
Odessa Astronomical Publications, 2017 Space density distributions of meteoroids over the sphere with radius 1 AU and the centre in the Sun were found for meteoroid masses greater than 10-3 g, 10-2 g and 1 g.
O. I. Belkovich, S. L. Suleymanova
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Analysis of Moon impact flashes detected during the 2012 and 2013 Perseids [PDF]
, 2015 We present the results of our Moon impact flashes detection campaigns performed around the maximum activity period of the Perseid meteor shower in 2012 and 2013.
Ana-Hernández, Leonor +6 more
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The 2011 October Draconids Outburst. II. Meteoroid Chemical Abundances from Fireball Spectroscopy [PDF]
, 2013 On October 8, 2011 the Earth crossed dust trails ejected from comet 21P/Giacobini-Zinner in the late 19th and early 20th Century. This gave rise to an outburst in the activity of the October Draconid meteor shower, and an international team was organized
Cabrera-Caño, J. +6 more
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3D/Biela and the Andromedids: Fragmenting versus Sublimating Comets [PDF]
, 2007 Comet 3D/Biela broke up in 1842/1843 and continued to disintegrate in the returns of 1846 and 1852. When meteor storms were observed in November of 1872 and 1885, it was surmised that those showers were the debris from that breakup.
Jenniskens, P., Vaubaillon, J.
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Astronomy & Astrophysics, 2019 Context.A significant fraction of small meteors are produced by iron meteoroids. Their origin and the interaction with the atmosphere have not been well explained up to now.Aims.The goals of the study are to observe faint, slow, low altitude meteors, to identify candidates for iron meteoroids among them, to model their ablation and light curves, and to
David Čapek +5 more
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