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相关论文: Comet C/2011 L4 (PanStarrs): Small nucleus, fast r…

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During its sungrazing perihelion passage, comet ISON appeared in the field of view of the SUMER spectrometer and allowed unique observations at far-ultraviolet wavelengths with high spatial and temporal resolution. We report results of…

太阳与恒星天体物理 · 物理学 2015-06-22 W. Curdt , H. Boehnhardt , J. -B. Vincent , S. K. Solanki , U. Schühle , L. Teriaca

Long-period comets are planetesimal remnants constraining the environment and volatiles of the protoplanetary disc. We report the discovery of hyperbolic long-period comet C/2022 E3 (ZTF), which has a perihelion $\sim$1.11 au, an…

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

New orbit for C/2014 W10 PANSTARRS is obtained. High original eccentricity of e = 1.65 might suggest an interstellar origin of this comet. The probable reasons for missing this possible important event is discussed and a call for searching…

地球与行星天体物理 · 物理学 2018-10-31 Piotr A. Dybczyński , Małgorzata Królikowska

The line emission in the coma was measured in the comets C/2001 Q4 (NEAT) and C/2002 T7 (LINEAR), that were observed on five consecutive nights, 7-11 May 2004, at heliocentric distances of 1.0 and 0.7 AU, respectively, by means of…

地球与行星天体物理 · 物理学 2013-11-11 M. de Val-Borro , M. Küppers , P. Hartogh , L. Rezac , N. Biver , D. Bockelée-Morvan , J. Crovisier , C. Jarchow , G. L. Villanueva

We present polarization images of Comet ISON (C/2012 S1) taken with the Hubble Space Telescope (HST) on UTC 2013 May 8 (rh = 3.81 AU, Delta = 4.34 AU), when the phase angle was alpha = 12.16 degrees. This phase angle is approximately…

Near-Earth asteroid 2012 DA14 made its closest approach on February 15, 2013, when it passed at a distance of 27,700 km from the Earth's surface. It was the first time an asteroid of moderate size was predicted to approach that close to the…

We present imaging and spectroscopic data on comet 19P/Borrelly that were obtained around the time of the Deep Space 1 encounter and in subsequent months. In the four months after perihelion, the comet showed a strong primary (sunward) jet…

天体物理学 · 物理学 2009-11-07 Tony L. Farnham , Anita L. Cochran

Comet C/2002 S2, a member of the Kreutz family of Sungrazing comets, was discovered in white light images of the SOHO/LASCO coronagraph on 2002 September 18 and observed in \hi\, \lya\, emission by the SOHO/UVCS instrument at four different…

太阳与恒星天体物理 · 物理学 2015-06-23 Silvio Giordano , John C. Raymond , Philippe Lamy , Michael Uzzo , Danuta Dobrzycka

We present an analysis of the photometric and spectroscopic data of the comet C/2012 S1 (ISON) observed at the heliocentric distances of 6.21\div 4.81 AU. The photometric observations were made with the 60-cm Zeiss-600 telescope (ICAMER,…

Comet 12P/Pons-Brooks is a periodic comet with an orbital period of approximately 71 years. Because of the period duration, aphelion of 35.3 au, and highly inclined orbit (74.2 deg), it is classified as a Halley-type comet. In this work, we…

We present the results of a global coma morphology campaign for comet C/2012 S1 (ISON), which was organized to involve both professional and amateur observers. In response to the campaign, many hundreds of images, from nearly two dozen…

地球与行星天体物理 · 物理学 2015-12-23 Nalin H. Samarasinha , 48 co-authors

We report the recovery of returning Halley-type comet 12P/Pons-Brooks using the 4.3 m Lowell Discovery Telescope, at a heliocentric distance of 11.89 au. Comparative analysis with a dust model suggests that the comet may have been active…

地球与行星天体物理 · 物理学 2020-07-06 Quanzhi Ye , Tony L. Farnham , Matthew M. Knight , Carrie E. Holt , Lori M. Feaga

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 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

Comet C/2017 K2 (Pan-STARRS) provided a rare opportunity to investigate the evolution of coma composition and outgassing patterns over a transitional heliocentric distance (Rh) range where activity drivers in comets are thought to change…

Spectra of comet C/2014 Q2 (Lovejoy) were taken with a low resolution spectrograph mounted on the 0.5 m telescope at the Mount Abu Infrared Observatory (MIRO), India during January to May 2015 covering the perihelion and post-perihelion…

地球与行星天体物理 · 物理学 2016-09-27 Kumar Venkataramani , Satyesh Ghetiya , Shashikiran Ganesh , U. C. Joshi , Vikrant K. Agnihotri , K. S. Baliyan

We report observations of comet C/2014 UN271 (Bernardinelli-Bernstein) carried out on UT 2024 March 8 and 17 at a heliocentric distance ($r_{\mathrm{H}}$) of 16.6 au using the Atacama Large Millimeter/Submillimeter Array (ALMA). The CO…

The chance discovery of the first interstellar minor body, 1I/2017 U1 (`Oumuamua), indicates that we may have been visited by such objects in the past and that these events may repeat in the future. Unfortunately, minor bodies following…

地球与行星天体物理 · 物理学 2019-08-30 C. de la Fuente Marcos , R. de la Fuente Marcos

The results of the photometric observations of comet C/2009 P1 (Garradd) performed at the 60-cm Zeiss-600 telescope of the Terskol observatory have been analyzed. During the observations, the comet was at the heliocentric and geocentric…

地球与行星天体物理 · 物理学 2021-01-15 A. V. Ivanova , S. A. Borisenko , M. V. Andreev