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相关论文: Preview of Comet C/2021 A1 (Leonard) and Its Encou…

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We present the results of a molecular survey of long period comets C/2021 A1 (Leonard) and C/2022 E3 (ZTF). Comet C/2021 A1 was observed with the IRAM 30-m radio telescope in November-December 2021 before perihelion when it was closest to…

Comet C/2013 A1 (Siding Spring) will have a close encounter with Mars on October 19, 2014. We model the dynamical evolution of dust grains from the time of their ejection from the comet nucleus to the Mars close encounter, and determine the…

Comet C/2013 A1 (siding Spring) will experience a high velocity encounter with Mars on October 19, 2014 at a distance of 135,000 km +- 5000 km from the planet center. We present a comprehensive analysis of the trajectory of both the comet…

地球与行星天体物理 · 物理学 2015-06-19 Davide Farnocchia , Steven R. Chesley , Paul W. Chodas , Pasquale Tricarico , Michael S. P. Kelley , Tony L. Farnham

We present imaging observations of the disintegrating long-period comet C/2021 A1 (Leonard). High resolution observations with Hubble Space Telescope show no evidence for surviving fragments, and place a 3 sigma upper limit to their…

地球与行星天体物理 · 物理学 2023-05-19 David Jewitt , Yoonyoung Kim , Michael Mattiazzo , Max mutchler , Jing Li , Jessica Agarwal

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

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…

Although the nucleus of comet C/2013 A1 (Siding Spring) will safely pass Mars in October 2014, the dust in the coma and tail will more closely approach the planet. Using a dynamical model of comet dust, we estimate the impact fluence. Based…

地球与行星天体物理 · 物理学 2015-06-22 Michael S. P. Kelley , Tony L. Farnham , Dennis Bodewits , Pasquale Tricarico , Davide Farnocchia

We report a pre-perihelion survey of volatile emissions from comet D/2021 A1 (Leonard) with the Northern Extended Millimeter Array (NOEMA; UT 2021 Nov. 5, 21, and Dec. 1) and the Atacama Pathfinder Experiment (APEX; UT 2021 Dec. 9-10),…

In this paper, we present a unique data set of more than one year's worth of regular observations of comet C/2013 A1(Siding Spring) with TRAPPIST in Chile, along with low-resolution spectra obtained with the ESO/VLT FORS 2 instrument. The…

地球与行星天体物理 · 物理学 2016-04-20 C. Opitom , A. Guilbert-Lepoutre , E. Jehin , J. Manfroid , D. Hutsemékers , M. Gillon , P. Magain , G. Roberts-Borsani , O. Witasse

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 Object Wide-field Infrared Survey Explorer (NEOWISE) mission observed comet C/2013 A1 (Siding Spring) three times at 3.4 {\mu}m and 4.6 {\mu}m as the comet approached Mars in 2014. The comet is an extremely interesting target…

地球与行星天体物理 · 物理学 2015-06-23 R. Stevenson , J. M. Bauer , R. M. Cutri , A . K. Mainzer , F. J. Masci

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

We show that the estimates of close encounter of this comet with Mars depend on data treatment. Using the data taken in the two-year period, we derived that the comet will miss Mars on 2014 October 19 at the distance of about $140\,150\pm…

空间物理 · 物理学 2014-10-08 Paweł Wajer , Małgorzata Królikowska

A stable population of objects co-orbiting with Venus was recently hypothesized in order to explain the existence of Venus's co-orbital dust ring. We conducted a 5 day twilight survey for these objects with the Cerro-Tololo Inter-American…

地球与行星天体物理 · 物理学 2020-08-06 Petr Pokorny , Marc J. Kuchner , Scott S. Sheppard

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

We present observations of comet 67P/Churyumov-Gerasimenko during its 2021/22 apparition, aiming to investigate its dust and gas environment and compare the results with those obtained in 2015/16 using the same telescope. Quasi-simultaneous…

地球与行星天体物理 · 物理学 2025-09-17 V. Rosenbush , V. Kleshchonok , O. Ivanova , I. Luk'yanyk , C. Snodgrass , D. Gardener , L. Kolokolova , J. Markkanen , E. Shablovinskaya

We present a deep imaging and spectroscopic search for emission from (3200) Phaethon, a large near-Earth asteroid that appears to be the parent of the strong Geminid meteoroid stream, using the 4.3 m Lowell Discovery Telescope. Observations…

地球与行星天体物理 · 物理学 2020-11-23 Quanzhi Ye , Matthew M. Knight , Michael S. P. Kelley , Nicholas A. Moskovitz , Annika Gustafsson , David Schleicher

We observed comet C/2025 A6 with the Five-hundred-meter Aperture Spherical radio Telescope (FAST) equipped with the ultra-wideband receiver from 2025 October 23 to November 8, and it was the first detection for this comet with FAST.Through…

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

On 4 March 2021 at 9 UTC a 30-m in diameter near-Earth asteroid 2021 DW1 passed the Earth at a distance of 570000 km, reaching the maximum brightness of V=14.6 mag. We observed it photometrically from 2 March, when it was visible at V=16.5…

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