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相关论文: Frozen to death? -- Detection of comet Hale-Bopp a…

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Eleven years after its perihelion, comet C/1995 O1 (Hale-Bopp) is still active. Between October 20--22, 2007, we detected a diffuse coma of 180x10^3$km in diameter with a slight elongation toward N/S direction. The integrated brightness was…

天体物理学 · 物理学 2009-11-13 Gy. M. Szabo , L. L. Kiss , K. Sarneczky

Here we report that the activity of comet Hale--Bopp ceased between late 2007 and March, 2009, at about 28 AU distance from the Sun. At that time the comet resided at a distance from the Sun that exceeded the freeze-out distance of regular…

地球与行星天体物理 · 物理学 2015-06-11 Gy. M. Szabó , L. L. Kiss , A. Pál , Cs. Kiss , K. Sárneczky , A. Juhász , M. R. Hogerheijde

Conventional narrowband photoelectric photometry of Comet Hale-Bopp (1995 O1) was obtained on 99 nights from mid-1995 to early-2000, yielding gas and dust production rates over an unprecedented range of time and distance. The appearance of…

地球与行星天体物理 · 物理学 2024-09-23 David G. Schleicher , Peter V. Birch , Tony L. Farnham , Allison N. Bair

Comet C/1995 O1 (Hale-Bopp) has provided an unprecedented opportunity to observe a bright comet over a wide range of heliocentric distances. We present here Spitzer Space Telescope observations of Hale-Bopp from 2005 and 2008 that show a…

地球与行星天体物理 · 物理学 2014-04-10 Emily A. Kramer , Yanga R. Fernandez , Carey M. Lisse , Michael S. Kelley , Laura M. Woodney

Observations of the CO J(1-0) 115 GHz and J(2-1) 230 GHz lines in comet C/1995 O1 (Hale-Bopp) were performed with the IRAM Plateau de Bure interferometer on 11 March, 1997. The observations were conducted in both single-dish (ON-OFF) and…

地球与行星天体物理 · 物理学 2010-11-02 D. Bockelée-Morvan , F. Henry , N. Biver , J. Boissier , P. Colom , J. Crovisier , D. Despois , R. Moreno , J. Wink

On 2007 October 29 the outbursting comet 17P/Holmes passed within 0.79 arcsec of a background star. We recorded the event using optical, narrowband photometry and detect a 3% to 4% dip in stellar brightness bracketing the time of closest…

地球与行星天体物理 · 物理学 2015-06-11 Pedro Lacerda , David Jewitt

Based on long-slit infrared spectroscopic observations, it has been suggested that half of the carbon monoxide present in the atmosphere of comet C/1995 O1 (Hale-Bopp) close to perihelion was released by a distributed source in the coma,…

地球与行星天体物理 · 物理学 2015-05-19 D. Bockelée-Morvan , J. Boissier , N. Biver , J. Crovisier

Activity of most comets near the Sun is dominated by sublimation of frozen water, the most abundant ice in comets. Some comets, however, are active well beyond the water-ice sublimation limit of ~3 AU. Three bodies dominate the…

地球与行星天体物理 · 物理学 2017-03-23 Maria Womack , Gal Sarid , Kacper Wierzchos

The long-term brightness evolution of the great comet C/1995 O1 (Hale-Bopp) presented a remarkable opportunity to study the behavior of its coma over four years. We used approximately 2200 total visual magnitudes published in the…

The prime objective is to settle a contradiction between a high nongravitational acceleration affecting the orbital motion of comet C/1995 O1 and its enormous nucleus by modeling it as a compact cluster of boulder-sized fragments held…

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

On 30.14 March 1997 we observed the EUV spectrum of the bright comet C/1995 O1 (Hale-Bopp) at the time of its perihelion, using our EUVS sounding rocket telescope/spectrometer. The spectra reveal the presence H Ly beta, O+, and, most…

On 2018 November 18, coronagraphs onboard the Solar and Heliospheric Observatory (SOHO) captured an unrecognized comet crossing its fields of view. We identified this comet to be the minor planet (139359) 2001 ME1 whose previously unnoticed…

地球与行星天体物理 · 物理学 2026-02-09 Qicheng Zhang , Quanzhi Ye , Karl Battams , Matthew M. Knight , Worachate Boonplod , Rainer Kracht

We report the discovery of X-ray emission from comet C/1995 O1 (Hale-Bopp) by the LECS instrument on-board BeppoSAX on 1996 September 10--11. The 0.1--2.0 keV luminosity decayed by a factor of 2 on a timescale of ~10 hr with a mean value of…

We present observations showing in-bound long-period comet C/2017 K2 (PANSTARRS) to be active at record heliocentric distance. Nucleus temperatures are too low (60 K to 70 K) either for water ice to sublimate or for amorphous ice to…

地球与行星天体物理 · 物理学 2017-10-04 David Jewitt , Man-To Hui , Max Mutchler , Harold Weaver , Jing Li , Jessic Agarwal

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 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

The outburst and subsequent brightness evolution of Comet 17P/Holmes has been observed using the MMT Observatory's All-Sky Camera (Pickering 2006) on Mt. Hopkins near Tucson, Arizona, USA. The comet was picked up at the limiting visual…

地球与行星天体物理 · 物理学 2010-09-02 E. E. El-Houssieny , R. J. Nemiroff , T. E. Pickering

We present a high-resolution observation of distant comet C/2014 UN$_{271}$ (Bernardinelli-Bernstein) using the {\it Hubble Space Telescope} on 2022 January 8. The signal of the nucleus was successfully isolated by means of the nucleus…

地球与行星天体物理 · 物理学 2022-04-20 Man-To Hui , David Jewitt , Liang-Liang Yu , Max J. Mutchler

We report results from broadband visible images of comet C/2012 S1 (ISON) obtained with the Hubble Space Telescope Wide Field Camera 3 on 2013 April 10. C/ISON's coma brightness follows a 1/{\rho} (where {\rho} is the projected distance…

Remote investigations of the ancient solar system matter has been traditionally carried out through the observations of long-period (LP) comets that are less affected by solar irradiation than the short-period counterparts orbiting much…

地球与行星天体物理 · 物理学 2016-12-14 K. Sarneczky , Gy. M. Szabo , B. Csak , J. Kelemen , G. Marschalko , A. Pal , R. Szakats , T. Szalai , E. Szegedi-Elek , P. Szekely , K. Vida , J. Vinko , L. L. Kiss
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