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相关论文: Orbital Elements of Comet C/1490 Y1 and the Quadra…

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The asteroid 2003 EH1, proposed as the parent body of the Quadrantid meteor shower, is thought to be the remnant of a past cometary object, tentatively identified with the historical comets C/1490 Y1 and C/1385 U1. In the present work we…

天体物理学 · 物理学 2009-09-02 Marco Micheli , Fabrizio Bernardi , David J. Tholen

The Quadrantid meteor shower is among the strongest annual meteor showers, and has drawn the attention of scientists for several decades. The stream is unusual, among others, for several reasons: its very short duration around maximum…

地球与行星天体物理 · 物理学 2015-09-16 Abedin Abedin , Pavel Spurny , Paul Wiegert , Petr Pokorny , Jiri Borovicka , Peter Brown

Sungrazing comets have always captured a lot of interest and curiosity among the general public as well as scientists since ancient times. The perihelion passage of comet C/2012 S1 (ISON) at the end of this year (on 2013 November 28) is an…

地球与行星天体物理 · 物理学 2015-06-17 A. Sekhar , D. J. Asher

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

An analysis is presented for the photometric data on comet C/2013 A1 (Siding Spring) from observations at a large heliocentric distance (near 4.1 AU). Comet C/2013 A1 (Siding Spring) displays intense activity despite the relatively large…

地球与行星天体物理 · 物理学 2020-12-23 Yu. S. Andrienko , A. V. Golovin , A. V. Ivanova , V. N. Reshetnik , S. N. Kolesnik , S. A. Borisenko

The near-Earth asteroid (196256) 2003 EH1 has been suggested to have a dynamical association with the Quadrantid meteoroid stream. We present photometric observations taken to investigate the physical character of this body and to explore…

地球与行星天体物理 · 物理学 2015-10-28 Toshihiro Kasuga , David Jewitt

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

The thermal emission of comet C/2013 A1 (Siding Spring) was observed on March 31, 2013, at a heliocentric distance of 6.48 au using the PACS photometer camera of the Herschel Space Observatory. The comet was clearly active, showing a coma…

地球与行星天体物理 · 物理学 2015-01-21 Cs. Kiss , T. G. Müller , M. Kidger , P. Mattisson , G. Marton

C/1890 F1 Brooks belongs to a group of nineteen comets used by Jan Oort to support his famous hypothesis on the existence of a spherical cloud containing hundreds of billions of comets with orbits of semimajor axes between 50 and 150…

地球与行星天体物理 · 物理学 2016-05-25 Małgorzata Królikowska , Piotr A. Dybczyński

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

We used the UltraViolet-Optical Telescope on board Swift to systematically follow the dynamically new comet C/2013 A1 (Siding Spring) on its approach to the Sun. The comet was observed from a heliocentric distance of 4.5 AU pre-perihelion…

地球与行星天体物理 · 物理学 2015-06-24 Dennis Bodewits , Michael S. P. Kelley , Jian-Yang Li , Tony L. Farnham , Michael F. A'Hearn

We study a potential genetic relationship of comets C/1846 O1 and C/1973 D1, whose apparent orbital similarity was tested by Kresak (1982) only statistically, using the Southworth-Hawkins (1963) criterion D. Our orbit determination for…

地球与行星天体物理 · 物理学 2016-07-13 Zdenek Sekanina , Rainer Kracht

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

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

This comprehensive study of comet C/1995 O1 focuses first on investigating its orbital motion over a period of 17.6 yr (1993-2010). The comet is suggested to have approached Jupiter to 0.005 AU on -2251 November 7, in general conformity…

地球与行星天体物理 · 物理学 2017-09-12 Zdenek Sekanina , Rainer Kracht

The close encounter of Comet C/2013 A1 (Siding Spring) with Mars on October 19, 2014 presented an extremely rare opportunity to obtain the first flyby quality data of the nucleus and inner coma of a dynamically new comet. However, the…

Long period comet C/2021 A1 (Leonard) will approach Venus to within 0.029 au on 2021 December 18 and may subsequently graze the planet with its dust trail less than two days later. We observed C/2021 A1 with the Lowell Discovery Telescope…

地球与行星天体物理 · 物理学 2021-10-19 Qicheng Zhang , Quanzhi Ye , Shreyas Vissapragada , Matthew M. Knight , Tony L. Farnham

The dynamically new comet, C/2013 A1 (Siding Spring), is to make a close approach to Mars on 2014 October 19 at 18:30 UT at a distance of 40+/-1 Martian radius. Such extremely rare event offers a precious opportunity for the spacecrafts on…

地球与行星天体物理 · 物理学 2015-06-19 Quan-Zhi Ye , Man-To Hui

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

C/2002 CE$_{10}$ is an object in a retrograde elliptical orbit with Tisserand parameter $-0.853$ indicating a likely origin in the Oort Cloud. It appears to be a rather inactive comet since no coma and only a very weak tail was detected…

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