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相关论文: Meteor Shower Modeling: Past and Future Draconid O…

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The October Draconid meteor shower, produced by comet 21P/Giacobini-Zinner, is notorious for rare but intense outbursts, some exceeding rates of about 10 000 meteors per hour. In 2025, Earth will encounter young trails ejected by the comet…

地球与行星天体物理 · 物理学 2025-10-01 Auriane Egal , Paul Wiegert , Danielle E. Moser , Peter G. Brown , Margaret Campbell-Brown

Predictions of the 2018 Draconid activity at the Earth and the Sun-Earth L1 and L2 Lagrange points are presented. Numerical simulations of the meteoroids' ejection and evolution from comet 21P/Giacobini-Zinner are performed with a careful…

地球与行星天体物理 · 物理学 2018-10-17 Auriane Egal , Paul Wiegert , Peter G. Brown , Danielle E. Moser , Althea V. Moorhead , William J. Cooke

We present the results of a long term telescopic observation campaign of comet 21P/Giacobini-Zinner, parent body of the Draconid meteor shower, spanning $\sim 240$ days during its 2018 apparition. Determinations of comet 21P's dust…

地球与行星天体物理 · 物理学 2019-06-19 Steven Ehlert , Natalie Moticska , Auriane Egal

An unexpected intense outburst of the Draconid meteor shower was detected by the Canadian Meteor Orbit Radar (CMOR) on October 8, 2012. The peak flux occurred at ~16:40 UT on October 8 with a maximum of 2.4 +/- 0.3 hr-1 km-2 (appropriate to…

地球与行星天体物理 · 物理学 2015-06-17 Quanzhi Ye , Paul A. Wiegert , Peter G. Brown , Margaret D. Campbell-Brown , Robert J. Weryk

On October 8th, 2011 the Earth crossed the dust trails left by comet 21P/Giacobini-Zinner during its XIX and XX century perihelion approaches with the comet being close to perihelion. The geometric circumstances of that encounter were thus…

During the 2011 outburst of the Draconid meteor shower, members of the Video Meteor Network of the International Meteor Organization (IMO) provided, for the first time, fully automated flux density measurements in the optical domain. The…

地球与行星天体物理 · 物理学 2015-06-18 Sirko Molau , Geert Barentsen

A new meteor shower $\lambda$-Sculptorids produced by the comet 46P/Wirtanen was forecast for December 12, 2023. The predicted activity was highly uncertain, but generally considered to be low. Observations in Australia, New Zealand, and…

地球与行星天体物理 · 物理学 2024-02-13 D. Vida , J. M. Scott , A. Egal , J. Vaubaillon , Q. -Z. Ye , D. Rollinson , M. Sato , D. E. Moser

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…

地球与行星天体物理 · 物理学 2015-06-15 J. M. Madiedo , J. M. Trigo-Rodriguez , N. Konovalova , I. P. Williams , A. J. Castro-Tirado , J. L. Ortiz , J. Cabrera-Caño

Context. Several authors predicted an outburst of the Draconid meteor shower in 2018, but with an uncertain level of activity. Aims. Optical meteor observations were used to derive the population and mass indices, flux, and radiant…

地球与行星天体物理 · 物理学 2020-04-01 Denis Vida , Margaret Campbell-Brown , Peter G. Brown , Auriane Egal , Michael J. Mazur

A tau-Herculid meteor outburst or even a storm was predicted by several models to occur around 5~UT on 31~May, 2022 as a consequence of the break-up of comet 73P/Schwassmann-Wachmann 3 in 1995. The multi-instrument and multi-station…

A strong outburst of the October Draconid meteor shower was predicted for October 8, 2011. Here we present the observations obtained by the Canadian Meteor Orbit Radar (CMOR) during the 2011 outburst. CMOR recorded 61 multi-station Draconid…

地球与行星天体物理 · 物理学 2015-06-15 Quanzhi Ye , Peter G. Brown , Margaret D. Campbell-Brown , Robert J. Weryk

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…

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 Draconid meteor shower shows strong bursts of activity at irregular intervals, with nearly no activity in intervening years. Five outbursts of the Draconid meteor shower were observed with specular meteor radars in Canada and Europe…

地球与行星天体物理 · 物理学 2021-07-27 M. D. Campbell-Brown , G. Stober , C. Jacobi , J. Kero , A. Kozlovsky , M. Lester

We present ground-based optical and Spitzer Space Telescope infrared imaging observations of the ecliptic (Jupiter-family) comet 21P/Giacobini-Zinner, the parent body of the Draconid meteor stream, during its 2005 apparition. Onset of…

天体物理学 · 物理学 2009-11-13 Jana Pittichova , Charles E. Woodward , Michael S. Kelley , William T. Reach

We have carried out a continuous multi-band photometric monitoring of the nuclear activity of comet 29P/Schwassmann-Wachmann 1 from 2008 to 2010. Our main aim has been to study the outburst mechanism on the basis of a follow-up of the…

After the prediction of meteor showers in the Earth's atmosphere caused by the particles originating in the nucleus of comet 21P/Giacobini-Zinner, we went on with the prediction of showers on the other three terrestrial planets. Based on…

地球与行星天体物理 · 物理学 2023-08-09 Dušan Tomko , Luboš Neslušan

The massive outburst of the comet 17P/Holmes in October 2007 is the largest known outburst by a comet thus far. We present a new comprehensive model describing the evolution of the dust trail produced in this phenomenon. The model comprises…

地球与行星天体物理 · 物理学 2022-05-10 Maria Gritsevich , Markku Nissinen , Arto Oksanen , Jari Suomela , Elizabeth A. Silber

Context. The existence of meteor clusters has long since been a subject of speculation and so far only seven events have been reported, among which two involve less than five meteors, and three were seen during the Leonid storms. Aims. The…

The Ursid meteor shower is an annual shower that usually shows little activity. However, its Zenith Hourly Rate sometimes increases, usually either when its parent comet, 8P/Tuttle, is close to its perihelion or its aphelion. Outbursts when…

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