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相关论文: Long-term outburst activity of comet 17P/Holmes an…

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Context. On October 24, 2007 the periodic comet 17P/Holmes underwent an astonishing outburst that increased its apparent total brightness from magnitude V\sim17 up to V\sim2.5 in roughly two days. We report on Wendelstein 0.8 m telescope…

天体物理学 · 物理学 2009-11-13 M. Montalto , A. Riffeser , U. Hopp , S. Wilke , G. Carraro

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

Comet 17P/Holmes underwent the largest cometary outburst in recorded history on UT 2007 Oct. 23, releasing massive quantities of dust and gas. We used the Canada-France-Hawaii telescope to obtain wide-field images of 17P/Holmes on 15 dates…

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

Comet 17P/Holmes underwent a dramatic outburst in October 2007, caused by the sudden fragmentation of its nucleus and the production of a large quantity of grains scattering sunlight. We report on 90 GHz continuum observations carried out…

地球与行星天体物理 · 物理学 2015-06-05 J. Boissier , D. Bockelée-Morvan , N. Biver , J. Crovisier , E. Lellouch , R. Moreno , V. Zakharov

A Jupiter-family comet, 17P/Holmes, underwent outbursts in 1892 and 2007. In particular, the 2007 outburst is known as the greatest outburst over the past century. However, little is known about the activity before the outburst because it…

We present time-resolved photometric observations of Jupiter family comet 17P/Holmes during its dramatic outburst of 2007. The observations, from the orbiting Solar Mass Ejection Imager (SMEI), provide the most complete measure of the…

地球与行星天体物理 · 物理学 2015-05-20 Jing Li , David Jewitt

Comet 17P/Holmes underwent a massive outburst in 2007 Oct., brightening by a factor of almost a million in under 48 hours. We used infrared images taken by the Wide-Field Survey Explorer mission to characterize the comet as it appeared at a…

地球与行星天体物理 · 物理学 2015-06-19 R. Stevenson , J. M. Bauer , E. A. Kramer , T. Grav , A. K. Mainzer , J. R. Masiero

An explosion on comet 17P/Holmes occurred on 2007 Oct 23, projecting particulate debris of a wide range of sizes into the interplanetary medium. We observed the comet using the Spitzer spectrograph on 2007 Nov 10 and 2008 Feb 27, and the…

地球与行星天体物理 · 物理学 2015-05-18 William T. Reach , Jeremie Vaubaillon , Carey M. Lisse , Mikel Holloway , Jeonghee Rho

This paper reports a new optical observation of 17P/Holmes one orbital period after the historical outburst event in 2007. We detected not only a common dust tail near the nucleus, but also a long narrow structure that extended along the…

We present wide-field imaging of the 2007 outburst of Comet 17P/Holmes obtained serendipitously by SuperWASP-North on 17 nights over a 42-night period beginning on the night (2007 October 22-23) immediately prior to the outburst. Photometry…

地球与行星天体物理 · 物理学 2015-05-19 Henry H. Hsieh , Alan Fitzsimmons , Yogesh Joshi , Damian Christian , Don L. Pollacco

We present results from a wide-field imaging campaign at the Canada-France-Hawaii Telescope to study the spectacular outburst of comet 17P/Holmes in late 2007. Using image-processing techniques we probe inside the spherical dust coma and…

地球与行星天体物理 · 物理学 2015-05-18 Rachel Stevenson , Jan Kleyna , David Jewitt

Based on millimeter-wavelength continuum observations we suggest that the recent 'spectacle' of comet 17P/Holmes can be explained by a thick, air-tight dust cover and the effects of H2O sublimation, which started when the comet arrived at…

地球与行星天体物理 · 物理学 2009-01-20 W. J. Altenhoff , E. Kreysa , K. M. Menten , A. Sievers , C. Thum , A. Weiss

We present high angular resolution Submillimeter Array observations ofthe outbursting Jupiter family comet 17P/Holmes on 2007 October 26-29, achieving a spatial resolution of 2.5", or ~3000 km at the comet distance. The observations…

地球与行星天体物理 · 物理学 2015-06-23 Chunhua Qi , Michiel R. Hogerheijde , David Jewitt , Mark A. Gurwell , David J. Wilner

During its most recent return, comet 12P/Pons-Brooks experienced 14 well-documented outbursts, observed between June 13, 2023, and April 2024, at heliocentric distances ranging from $4.26\,$au to $0.85\,$au. After perihelion, two additional…

地球与行星天体物理 · 物理学 2025-02-06 Maria Gritsevich , Marcin Wesołowski , Alberto J. Castro-Tirado

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

Outbursts are known to begin with a sudden appearance and steep brightening of a "stellar nucleus" --- an unresolved image of a plume of material on its way from the comet's surface and an initial stage of an expanding halo of ejecta. Since…

地球与行星天体物理 · 物理学 2014-09-29 Zdenek Sekanina

Cometary activity is a manifestation of sublimation-driven processes at the surface of nuclei. However, cometary outbursts may arise from other processes that are not necessarily driven by volatiles. In order to fully understand nuclear…

We present follow-up observations of comet 17/P Holmes after its extreme outburst in brightness, which occurred end of October 2007. We obtained 58 V-band images of the comet between October 2007 and February 2008, using the…

地球与行星天体物理 · 物理学 2015-05-13 M. Mugrauer , M. M. Hohle , C. Ginski , M. Vanko , F. Freistetter

Jupiter family comet 17P/Holmes underwent a remarkable outburst on UT 2007 Oct. 24, in which the integrated brightness abruptly increased by about a factor of a million.We obtained near infrared (0.8 - 4.2 micron) spectra of 17P/Holmes on…

地球与行星天体物理 · 物理学 2009-11-13 Bin Yang , David Jewitt , Schelte J. Bus

A mechanism is proposed to explain the outburst of comet 17P/Holmes based on; (a) oxidation of water within the porous surface of the comet nucleus to form hydrogen peroxide (H2O2) through exposure to UV radiation, to energetic solar-wind…

天体物理学 · 物理学 2007-12-21 Richard Miles
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