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相关论文: Meteors And Showers A Millennium Ago

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We have compiled and analyzed historical Korean meteor and meteor shower records in three Korean official history books, Samguksagi which covers the three Kingdoms period (57 B.C -- A.D. 935), Goryeosa of Goryeo dynasty (A.D. 918 -- 1392),…

天体物理学 · 物理学 2009-11-10 Hong-Jin Yang , Changbom Park , Myeong-Gu Park

Meteor showers occur when streams of meteoroids originating from a common source intersect the Earth. There will be small dissimilarities between the direction of motion of different meteoroids within a stream, and these small differences…

地球与行星天体物理 · 物理学 2022-06-01 Althea V. Moorhead , Tiffany Clements , Denis Vida

Meteoroids of a low-inclination stream hit the Earth arriving from a direction near the ecliptic. The radiant area of stream like this is often divided into two parts: one is situated northward and the other southward of the ecliptic. In…

地球与行星天体物理 · 物理学 2023-07-05 L. Neslušan , T. J. Jopek , R. Rudawska , M. Hajduková , G. Kokhirova

This is an overview of recent research on meteors and the parent bodies from which they are produced. While many meteor showers result from material ejected by comets, two out of the three strongest annual showers (the Geminids and the…

地球与行星天体物理 · 物理学 2022-09-21 Toshihiro Kasuga , David Jewitt

Small bodies in the solar system are conventionally classified into asteroids and comets. However, it is recently found that a small number of objects can exhibit properties of both asteroids and comets. Some are more consistent with…

地球与行星天体物理 · 物理学 2018-12-05 Quan-Zhi Ye

NEOs come close to the Earth's orbit so that any dust ejected from them, might be seen as a meteor shower. Orbits evolve rapidly, so that a similarity of orbits at one given time is not suffcient to prove a relationship, orbital evolution…

地球与行星天体物理 · 物理学 2015-06-18 Tadeusz J. Jopek , Iwan P. Williams

In studies of the oldest solar system bodies - comets and asteroids - it is their fragments - meteoroids - that provide the most accessible planetary material for detailed laboratory analysis in the form of dust particles or meteorites.…

地球与行星天体物理 · 物理学 2020-07-22 Pavol Matlovič , Juraj Tóth

The objectives of this project are to predict new meteor showers associated with as many as possible known periodic comets and to find a generic relationship of some already known showers with these comets. For a potential parent comet, we…

地球与行星天体物理 · 物理学 2014-10-07 Lubos Neslusan , Maria Hajdukova , Dusan Tomko , Zuzana Kanuchova , Marian Jakubik

December Monocerotids and November Orionids are weak but established annual meteor showers active throughout November and December. Analysis of a high quality orbits subset of the SonotaCo video meteor database shows that the distribution…

地球与行星天体物理 · 物理学 2011-03-23 Peter Vereš , Leonard Kornoš , Juraj Tóth

By using an array of high-sensitivity CCD video devices and spectrographs, the activity of meteor events from the poorly-known $\rho$-Geminid meteoroid stream has been monitored during January 2012 and 2013. As a result of this research,…

地球与行星天体物理 · 物理学 2015-06-23 Jose M. Madiedo

Earth occasionally crosses the debris streams produced by comets and other active bodies in our solar system. These manifest meteor showers that provide an opportunity to explore these bodies without a need to visit them in-situ.…

地球与行星天体物理 · 物理学 2022-09-23 Quanzhi Ye , Peter Jenniskens

We present a multi-instrumental, multidecadal analysis of the activity of the Eta-Aquariid and Orionid meteor showers for the purpose of constraining models of 1P/Halley's meteoroid streams. The interannual variability of the showers' peak…

地球与行星天体物理 · 物理学 2020-08-19 A. Egal , P. G. Brown , J. Rendtel , M. Campbell-Brown , P. Wiegert

We present a new numerical model of the eta-Aquariid and Orionid meteor showers. The model investigates the origin, variability and age of the eta-Aquariid and Orionid apparitions from 1985 to the present day, in order to forecast their…

地球与行星天体物理 · 物理学 2020-10-14 Auriane Egal , Paul Wiegert , Peter G. Brown , Margaret Campbell-Brown , Denis Vida

The $\delta$-Cancrid meteoroid stream forms four active meteor showers which are observable on the Earth annually during January-February and August-September. The stream's definite parent comet has not been established. We performed a…

地球与行星天体物理 · 物理学 2024-10-31 G. I. Kokhirova , M. Zhang , X. -G. Li , A. I. Zhonmuhammadi , X. Liu

Comet 1P/Halley has the unique distinction of having a very comprehensive set of observational records for almost every perihelion passage from 240 B.C. This has helped to constrain theoretical models pertaining to its orbital evolution.…

地球与行星天体物理 · 物理学 2015-06-15 Aswin Sekhar , David J Asher

Meteor showers and their outbursts are the dominant source of meteoroid impact risk to spacecraft on short time scales. Meteor shower prediction models depend on historical observations to produce accurate forecasts. However, the current…

A meteor shower is a luminous phenomenon that takes place by the entry into the Earths atmosphere of a cascade of particles coming from a stream intersected by our planet in its orbit. Here we investigate the possibility of a description of…

统计力学 · 物理学 2007-10-29 Oscar Sotolongo-Costa , R. Gamez , F. Luzon , A. Posadas , Pablo Weigandt Beckmann

The Desert Fireball Network observed a significant outburst of fireballs belonging to the Southern Taurid Complex of meteor showers between October 27 and November 17, 2015. At the same time, the Cameras for Allsky Meteor Surveillance…

Using orbital integrations of particles ejected from Comet Halley's passages between 1404 BC and 240 BC, the authors investigate possible outbursts of the Orionids (twin shower of the Eta Aquariids) that may have been observed in the…

地球与行星天体物理 · 物理学 2020-02-21 J. H. Kinsman , D. J. Asher

No firm evidence has existed that the ancient Maya civilization recorded specific occurrences of meteor showers or outbursts in the corpus of Maya hieroglyphic inscriptions. In fact, there has been no evidence of any pre-Hispanic…

地球与行星天体物理 · 物理学 2017-07-27 J. H. Kinsman , D. J. Asher
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