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The $\tau$-Herculids (IAU shower number #61 TAH) is a minor meteor shower associated with comet 73P/Schwassmann-Wachmann 3, a Jupiter-Family comet that disintegrated into several fragments in 1995. As a consequence of the nucleus break-up,…

地球与行星天体物理 · 物理学 2023-06-07 Auriane Egal , Paul A. Wiegert , Peter G. Brown , Denis Vida

The Taurid Meteoroid Complex (TMC) is a broad stream of meteoroids that produces several annual meteor showers on Earth. If the linkage between these showers and 2P/Encke is at the centre of most TMC models, the small size and low activity…

地球与行星天体物理 · 物理学 2022-08-17 A. Egal , P. Wiegert , P. G. Brown

We report on photometry and high resolution spectroscopy of the chemically peculiar Jupiter-family Comet (hereafter JFC) 21P/Giacobini-Zinner. Comet 21P is a well known member of the carbon-chain depleted family but displays also a…

地球与行星天体物理 · 物理学 2020-08-12 Y. Moulane , E. Jehin , P. Rousselot , J. Manfroid , Y. Shinnaka , F. J. Pozuelos , D. Hutsemékers , C. Opitom , B. Yang , Z. Benkhaldoun

The Andromedid meteor shower underwent spectacular outbursts in 1872 and 1885, producing thousands of visual meteors per hour and described as `stars fell like rain' in Chinese records of the time. The shower originates from comet 3D/Biela…

地球与行星天体物理 · 物理学 2015-06-11 Paul A. Wiegert , Peter G. Brown , Robert J. Weryk , Daniel K. Wong

Context. Comet 46P/Wirtanen is a near-Earth object (NEO) for which no associated meteor shower has ever been reported. Aims. This study is aimed at improving our understanding of why there has been no observed shower activity for this NEO…

地球与行星天体物理 · 物理学 2023-12-06 Jeremie Vaubaillon , Qhanzhi Ye , Auriane Egal , Mikiya Sato , Danielle Moser

NASA's Meteoroid Environment Office (MEO) produces an annual meteor shower forecast in order to help spacecraft operators assess the risk posed by meteoroid streams. Previously, this forecast focused on the International Space Station and…

地球与行星天体物理 · 物理学 2019-04-16 Althea V. Moorhead , Auriane Egal , Peter G. Brown , Danielle E. Moser , William J. Cooke

We obtained extensive narrowband photoelectric photometry of Comet 21P/Giacobini-Zinner with observations spanning 33 years. The original data from 1985 (Schleicher et al. 1987) were re-reduced and are presented along with data from three…

地球与行星天体物理 · 物理学 2022-04-27 David G. Schleicher

Mathematical modelling has shown that activity of the Geminid meteor shower should rise with time, and that was confirmed by analysis of visual observations 1985--2016. We do not expect any outburst activity of the Geminid shower in 2017,…

地球与行星天体物理 · 物理学 2018-01-24 G. O. Ryabova , J. Rendtel

The encounter of the meteoric material from 73P/Schmassmann--Wachmann~3 produced during the comet's 1995 outburst in May 2022 provides a rare and valuable opportunity to understand a fragmenting comet. Here we explore various ejection…

地球与行星天体物理 · 物理学 2022-07-20 Quanzhi Ye , Jérémie Vaubaillon

During its most recent return, comet 12P/Pons-Brooks experienced 14 well-documented outbursts, observed between June 13, 2023, and April 2024, at heliocentric distances ranging from $4.26\,$au to $0.85\,$au. After perihelion, two additional…

地球与行星天体物理 · 物理学 2025-02-06 Maria Gritsevich , Marcin Wesołowski , Alberto J. Castro-Tirado

{The multiple outburst events of comet 12P/Pons-Brooks during its 2024 apparition offer a unique window into highly-active volatile releasing processes not observable during quiescent periods. We performed radio observations of comet…

地球与行星天体物理 · 物理学 2025-09-17 Juncen Li , Xian Shi , Jianchun Shi , Yuehua Ma , Bin Yang , Jian-Yang Li , Zexi Xing , Man-To Hui , Zhen Wang , Ruining Zhao

We have analyzed the meteor activity associated with meteoroids of fresh dust trails of Comet 209P/LINEAR, which produced an outburst of the Camelopardalid meteor shower (IAU code #451, CAM) in May 2014. With this aim, we have employed an…

Meteoroid streams can be complex structures shaped by the processes of their formation and subsequent orbital evolution. The first step of their understanding is mapping their current stage. We used precise data from the European Fireball…

地球与行星天体物理 · 物理学 2025-03-12 J. Borovicka , P. Spurny , L. Kotkova , S. Molau , D. Tomko , T. Weiland

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…

Previous studies have suggested that Comet 209P/LINEAR may produce strong me- teor activity on Earth on 2014 May 24; however, exact timing and activity level is difficult to estimate due to the limited physical observations of the comet.…

地球与行星天体物理 · 物理学 2015-06-17 Quanzhi Ye , Paul A. Wiegert

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

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

The Leonids show meteor storms in a period of 33 years, and known as one of the most active meteor showers. It has recently shown a meteor stream consisting of several narrow dust trails made by meteoroids ejected from a parent comet.…

天体物理仪器与方法 · 物理学 2015-06-11 Tsutomu T. Takeuchi , Shigetomo Shiki , Daisuke Miyamoto , Hideaki Fujiwara , Jun Kitazume , Yousuke Utsumi

We report the successful detection of the "Arid" Meteor Shower (IAU\#1130 ARD), predicted to emerge for the first time in 2021, using a publicly accessible YouTube live camera developed by us. This live camera, installed on the Subaru…

地球与行星天体物理 · 物理学 2026-01-12 Ichi Tanaka , Hitoshi Hasegawa , Toyokazu Uda , Mikiya Sato , Jun-ichi Watanabe , Masanobu Higashiyama

Outbursts are known to begin with a sudden appearance and steep brightening of a "stellar nucleus" --- an unresolved image of a plume of material on its way from the comet's surface and an initial stage of an expanding halo of ejecta. Since…

地球与行星天体物理 · 物理学 2014-09-29 Zdenek Sekanina