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相关论文: Coma Morphology, Numerical Modeling, and Productio…

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We present an analysis of simultaneous X-Ray and UV observations ofcomet C/2007 N3 (Lulin) taken on three days between January 2009 and March 2009 using the Swift observatory. For our X-ray observations, we used basic transforms to account…

地球与行星天体物理 · 物理学 2015-06-04 J. A. Carter , D. Bodewits , A. M. Read , S. Immler

We report optical imaging, optical and near-infrared polarimetry, and Spitzer mid-infrared spectroscopy of comet C/2007 N3 (Lulin). Polarimetric observations were obtained in R (0.676 micron) at phase angles from 0.44 degrees to 21 degrees…

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

We report on photometry and imaging of Comet 103P/Hartley 2 obtained at Lowell Observatory from 1991 through 2011. We acquired photoelectric photometry on two nights in 1991, four nights in 1997/98, and 13 nights in 2010/11. We observed a…

地球与行星天体物理 · 物理学 2015-06-05 Matthew M. Knight , David G. Schleicher

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…

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…

We report on narrowband CN imaging of Comet 103P/Hartley 2 obtained at Lowell Observatory on 39 nights from 2010 July until 2011 January. We observed two features, one generally to the north and the other generally to the south. The CN…

地球与行星天体物理 · 物理学 2015-05-27 Matthew M. Knight , David G. Schleicher

The recent close approach of comet C/2020 F3 (NEOWISE) allowed us to study the morphology of its inner coma. From the measurement of the dust ejection velocityon spiral structures expanding around the nucleus, we estimated a mean…

地球与行星天体物理 · 物理学 2021-09-07 F. Manzini , V. Oldani , P. Ochner , E. Barbotin , L. R. Bedin , R. Behrend , G. Fardelli

Comet C/2007 N3 (Lulin) was observed with the Japanese infrared satellite AKARI in the near-infrared at a post-perihelion heliocentric distance of 1.7 AU. Observations were performed with the spectroscopic (2.5--5.0 micron) and imaging…

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.…

Observations on comet C/2007 N3 (Lulin) were made at phase angles close to opposition ($1.7^{\circ}$ - $10^{\circ}$). Photometric observations were carried out during 2009 February 24-28, in the IHW blue and red continuum and $R$ broad band…

地球与行星天体物理 · 物理学 2015-05-20 U. C. Joshi , S. Ganesh , K. S. Baliyan

We observed dynamically new sungrazing comet ISON (C/2012 S1) extensively at Lowell Observatory throughout 2013 in order to characterize its behavior prior to perihelion. ISON had "typical" abundances for an Oort Cloud comet. Its dust…

地球与行星天体物理 · 物理学 2015-06-23 Matthew M. Knight , David G. Schleicher

We observed comet C/2007 N3 (Lulin) twice on UT 28 January 2009, using the UV grism of the Ultraviolet and Optical Telescope (UVOT) on board the Swift Gamma Ray Burst space observatory. Grism spectroscopy provides spatially resolved…

地球与行星天体物理 · 物理学 2015-05-20 D. Bodewits , G. L. Villanueva , M. J. Mumma , W. B. Landsman , J. A. Carter , A. M. Read

We present a photometric and dynamical study of comet C/2010 U3 (Boattini), which was seen active in prediscovery data as early as 2005 November at a new inbound record heliocentric distance $r_{\rm H} = 25.8$ au. Two outburst events around…

地球与行星天体物理 · 物理学 2019-04-17 Man-To Hui , Davide Farnocchia , Marco Micheli

We report on our extensive photometry and imaging of Comet 46P/Wirtanen during its 2018/19 apparition and use these data to constrain modeling of Wirtanen's activity. Narrowband photometry was obtained on nine epochs from 2018 October…

地球与行星天体物理 · 物理学 2021-03-26 Matthew M. Knight , David G. Schleicher , Tony L. Farnham

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

Comet C/2006 W3 (Christensen) was observed in November 2009 at 3.3 AU from the Sun with Herschel. The PACS instrument acquired images of the dust coma in 70- and 160-micrometers filters, and spectra covering several H2O rotational lines.…

We analyze jet features found in the coma of Comet 21P/Giacobini-Zinner (21P/GZ) during its 2018 perihelion passage using narrowband CN photometric imaging in order to determine the comet's rotational period, and constrain the CN gas…

地球与行星天体物理 · 物理学 2023-01-19 Charles Goldberg , Cassandra Lejoly , Nalin Samarasinha

We reported the monitoring results on spectrophotometry, photometry and imaging of comet 103P/Hartley 2 obtained at Lulin (1m), Calar Alto (2.2m) and Beijing Astronomical (2.16m) Observatory from April to December 2010. We found that a dust…

太阳与恒星天体物理 · 物理学 2015-06-16 Zhong-Yi Lin , Luisa M. Lara , Wing-Huen Ip

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
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