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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

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

Eta-Virginids is a less-known meteor shower active in March. We investigated the meteoroids of this shower using fireball data from the European Fireball Network supplemented by video data of faint meteors. We first derived the criteria for…

地球与行星天体物理 · 物理学 2026-01-30 Jiri Borovicka , Pavel Spurny , Pavel Koten , Gabriel Borderes Motta , Lenka Kotkova , Rostislav Stork , Dusan Tomko , Thomas Weiland

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

Dormant comets in the near-Earth object (NEO) population are thought to be involved in the terrestrial accretion of water and organic materials. Identification of dormant comets is difficult as they are observationally indistinguishable…

地球与行星天体物理 · 物理学 2016-09-07 Quan-Zhi Ye , Peter G. Brown , Petr Pokorný

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

Meteorites provide an important source of information about the formation and composition of asteroids, because the level of accuracy of studies and analyses performed in a laboratory cannot be achieved by any ground or space based…

地球与行星天体物理 · 物理学 2023-08-11 Albino Carbognani , Marco Fenucci

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…

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

We provide an overview of the observational properties of the four major Taurid showers, namely the Northern and Southern Taurids (#017 NTA and #002 STA), the Beta Taurids (#173 BTA) and the Zeta Perseids (#172 ZPE). Analysing more than two…

地球与行星天体物理 · 物理学 2022-02-23 A. Egal , P. G. Brown , P. Wiegert , Y. Kipreos

Among the near-Earth object (NEO) population there are comets and active asteroids which are sources of fragments that initially move together; in addition, some NEOs follow orbits temporarily trapped in a web of secular resonances. These…

地球与行星天体物理 · 物理学 2016-01-05 C. de la Fuente Marcos , R. de la Fuente Marcos

The Geminids meteoroid stream produces one of the most intense meteor showers at Earth. It is an unusual stream in that its parent body is understood to be an asteroid, (3200) Phaethon, unlike most streams which are formed via ongoing…

地球与行星天体物理 · 物理学 2023-06-21 Wolf Z. Cukier , Jamey R. Szalay

Asteroid activity (e.g., thermo-mechanical breakdown, impacts, rotational shedding, tidal disruption, etc.) can inject meteoroids into near-Earth space and leave detectable signatures in orbit catalogs. We searched for such recent…

地球与行星天体物理 · 物理学 2026-02-20 Patrick M. Shober

Meteors can be classified into either sporadic meteors or showery meteors. We compile the meteor records in the astronomical archives in the Chronicle of the Koryo dynasty (918-1392), and investigate the spatial distribution of meteor…

天体物理学 · 物理学 2009-11-07 Sang-Hyeon Ahn

Taurid meteor shower produces prolonged but usually low activity every October and November. In some years, however, the activity is significantly enhanced. Previous studies based on long-term activity statistics concluded that the…

地球与行星天体物理 · 物理学 2017-09-13 P. Spurný , J. Borovička , H. Mucke , J. Svoreň

There is an unceasing incoming flux of extraterrestrial materials reaching the Earth's atmosphere. Some of these objects produce luminous columns when they ablate during the hypersonic encounter with air molecules. A few fireballs occur…

地球与行星天体物理 · 物理学 2024-05-29 E. Peña-Asensio , J. M. Trigo-Rodríguez , A. Rimola

Context. Orbital similarity measures, such as the D-values, have been extensively used in meteor science to identify meteoroid streams and associate meteorite falls with near-Earth objects (NEOs). However, the chaotic nature of near-Earth…

地球与行星天体物理 · 物理学 2024-12-25 Patrick M. Shober , Ariane Courtot , Jeremie Vaubaillon

We have made an extensive search for grouping amongst the near Earth asteroids (NEAs). We used two D- functions and rigorous cluster analysis approach. We have found sev- eral new groups (associations) among the NEAs: the objects moving on…

地球与行星天体物理 · 物理学 2020-03-04 Tadeusz J. Jopek
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