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相关论文: The rotation and coma profiles of comet C/2004 Q2 …

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Extensive observations of comet C/2004 Q2 (Machholz) were carried out between August 2004 and May 2005. The images obtained were used to investigate the comet's inner coma features at resolutions between 350 and 1500 km/pixel. A photometric…

This study presents findings from narrowband imaging of comet C/2006 P1 (McNaught) using the 3.6-metre New Technology Telescope (NTT) at La Silla, Chile. Observations commenced on January 27, 2007, 15 days after perihelion, and continued…

地球与行星天体物理 · 物理学 2026-03-03 Vincent Okoth , Cyrielle Opitom , Colin Snodgrass , Brian Murphy , James E. Robinson

We present results from CCD observations of comet 2P/Encke acquired at Steward Observatory's 2.3m Bok Telescope on Kitt Peak obtained in Oct. 2002, when the comet was near aphelion. Rotational lightcurves in B, V and R-filters were acquired…

天体物理学 · 物理学 2009-11-11 S. C. Lowry , P. R. Weissman

The results of the photometric observations of comet 29P/Schwassmann-Wachmann 1 are analyzed. The comet demonstrates substantial activity at heliocentric distances larger than 5 AU, outside the water ice sublimation zone. The CCD images of…

地球与行星天体物理 · 物理学 2020-12-17 A. V. Ivanova , V. L. Afanasiev , P. P. Korsun , A. R. Baranskii , M. V. Andreev , V. A. Ponomarenko

We observed comet C/2012 S1 (ISON) during six nights in February 2013 when it was at 4.8 AU from the sun. At this distance and time the comet was not very active and it was theoretically possible to detect photometric variations likely due…

The appearance of folding ion rays in cometary comae is still not very well understood, so our aim is to gain more insight into the role of the local solar wind in the formation of these structures. Comet C/2004 Q2 (Machholz) was…

天体物理学 · 物理学 2009-11-13 P. Degroote , D. Bodewits , M. Reyniers

We observed comet 96P/Machholz 1 on a total of 9 nights before and after perihelion during its 2017/2018 apparition. Both its unusually small perihelion distance and the observed fragmentation during multiple apparitions make 96P an object…

地球与行星天体物理 · 物理学 2019-05-01 Nora L. Eisner , Matthew M. Knight , Colin Snodgrass , Michael S. P. Kelley , Alan Fitzsimmons , Rosita Kokotanekova

We aim to determine the production rates of several parent and product volatiles and the 12C/13C isotopic carbon ratio in the long-period comet C/2004 Q2 (Machholz), which is likely to originate from the Oort Cloud. The line emission from…

地球与行星天体物理 · 物理学 2012-09-04 M. de Val-Borro , P. Hartogh , C. Jarchow , M. Rengel , G. L. Villanueva , M. Küppers , N. Biver , D. Bockelée-Morvan , J. Crovisier

Extensive observations of comet 260P (McNaught) were carried out between August 2012 and January 2013. The images obtained were used to analyze the inner coma morphology of the comet at resolutions ranging from 250 to about 1000 km/pixel. A…

地球与行星天体物理 · 物理学 2014-03-25 Federico Manzini , Virginio Oldani , Roberto Crippa , Jose' Borrero , Erik Bryssink , Martin Mobberley , Joel Nicolas , Sormano Obs

The CN coma structure of the EPOXI mission target, comet 103P/Hartley 2, was observed during twenty nights from September to December 2010. These CN images probe the rotational state of the comet's nucleus and provide a ground-based…

地球与行星天体物理 · 物理学 2015-05-28 Nalin H. Samarasinha , Beatrice E. A. Mueller , Michael F. A'Hearn , Tony L. Farnham , Alan Gersch

We report on photometry and imaging of Comet 10P/Tempel 2 obtained at Lowell Observatory from 1983 through 2011. We measured a nucleus rotation period of 8.950 +/- 0.002 hr from 2010 September to 2011 January. This rotation period is longer…

地球与行星天体物理 · 物理学 2015-06-11 Matthew M. Knight , David G. Schleicher , Tony L. Farnham , Edward W. Schwieterman , Samantha R. Christensen

High-dispersion (l/dl ~ 25,000) infrared spectra of Comet C/2004 Q2 (Machholz) were acquired on Nov. 28-29, 2004, and Jan. 19, 2005 (UT dates) with NIRSPEC at the Keck-2 telescope on Mauna Kea. We detected H2O, CH4, C2H2, C2H6, CO, H2CO,…

We present a measurement of the lifetime of ground state atomic carbon, C(^3P), against ionization processes in interplanetary space and compare it to the lifetime expected from the dominant physical processes likely to occur in this…

地球与行星天体物理 · 物理学 2015-05-20 Jeffrey P. Morgenthaler , Walter M. Harris , Michael R. Combi , Paul D. Feldman , Harold A. Weaver

Long period comet C/2014 B1 (Schwartz) exhibits a remarkable optical appearance, like that of a discus or bi-convex lens viewed edgewise. Our measurements in the four years since discovery reveal a unique elongated dust coma whose…

地球与行星天体物理 · 物理学 2019-02-20 David Jewitt , Yoonyoung Kim , Jane Luu , Ariel Graykowski

We observed Comet C/Siding Spring using the Hubble Space Telescope (HST) during its close approach to Mars. The high spatial resolution images obtained through the F689M, F775W, and F845M filters reveal the characteristics of the dust coma.…

We present CCD VR_C observations of 6 distant comets located at heliocentric distances of 3.4--7.2 AU. Time-series data were obtained on three nights in July, 2000 covering 16 hours. Each comet was observed after the perihelion, when a…

天体物理学 · 物理学 2009-11-06 Gy. Szabo , B. Csak , K. Sarneczky , L. L. Kiss

The nuclei of active comets emit molecules anisotropically from discrete vents. As the nucleus rotates, we expect to observe periodic variability in the molecular emission line profiles, which can be studied through mm/submm spectroscopy.…

We present R-band observations of comet C2004B1 obtained in the period June, 21 - August 20, 2006. The data have been reduced to surface brightness maps, light curves, and mean radial profiles of the coma. In two cases a decrease of the…

We summarize the collective knowledge of physical and surface properties of comet nuclei, focusing on those that are obtained from remote observations. We now have measurements or constraints on effective radius for over 200 comets,…

地球与行星天体物理 · 物理学 2023-04-20 Matthew M. Knight , Rosita Kokotanekova , Nalin H. Samarasinha

We analyzed images of comet 49P/Arend-Rigaux on 33 nights between 2012 January and May and obtained R-band lightcurves of the nucleus. Through usual phasing of the data we found a double-peaked lightcurve having a synodic rotation period of…

地球与行星天体物理 · 物理学 2017-10-25 Nora Eisner , Matthew M. Knight , David G. Schleicher
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