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We report photometric observations for comet C/2012 S1 (ISON) obtained during the time period immediately after discovery (r=6.28 AU) until it moved into solar conjunction in mid-2013 June using the UH2.2m, and Gemini North 8-m telescopes…

Comets and asteroids have long captured human curiosity, and until recently, all documented examples belonged to our Solar System. That changed with the discovery of the first known interstellar object, 1I/2017 U1 ('Oumuamua), in 2017. Two…

Earth and Planetary Astrophysics · Physics 2025-04-03 Josep M. Trigo-Rodríguez , Damya Souami , Maria Gritsevich , Marcin Wesołowski , Gennady Borisov

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…

Earth and Planetary Astrophysics · Physics 2015-06-23 Matthew M. Knight , David G. Schleicher

Centaurs are minor planets thought to have originated in the outer Solar System region known as the Kuiper Belt. Active Centaurs enigmatically display comet-like features (e.g., tails, comae) even though they orbit in the gas giant region…

Earth and Planetary Astrophysics · Physics 2020-04-15 Colin Orion Chandler , Jay K. Kueny , Chadwick A. Trujillo , David E. Trilling , William J. Oldroyd

A morphological and photometric analysis of the naked-eye long-period comet C/2022 E3 (ZTF) before perihelion is presented in this study. The observation images taken by the Zwicky Transient Facility survey telescope from July 2022 to…

Earth and Planetary Astrophysics · Physics 2024-05-27 Bin Liu , Xiaodong Liu

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…

We used the UltraViolet-Optical Telescope on board Swift to observe the dynamically young comet C/2009 P1 (Garradd) from a heliocentric distance of 3.5 AU pre-perihelion until 4.0 AU outbound. At 3.5 AU pre-perihelion, comet Garradd had one…

Earth and Planetary Astrophysics · Physics 2015-06-18 D. Bodewits , T. L. Farnham , M. F. A'Hearn , L. M. Feaga , A. McKay , D. G. Schleicher , J. M Sunshine

29P/Schwassmann-Wachmann 1 is a distant Centaur/comet, showing persistent CO-driven activity and frequent outbursts. We used the Herschel space observatory in 2010, 2011, and 2013 to observe H$_2$O and NH$_3$ and to image the dust coma.…

In 2017, 2018 and 2019, comets 46P/Wirtanen, 45P/Honda-Mrkos-Pajdusakova, and 41P/Tuttle-Giacobini-Kresak all had perihelion passages. Their hydrogen comae were observed by the Solar Wind ANisotropies (SWAN) all-sky hydrogen Lyman-alpha…

Earth and Planetary Astrophysics · Physics 2020-07-14 M. R. Combi , T. Mäkinen , J. -L. Bertaux , E. Quémerais , S. Ferron , R. Coronel

We report results based on mid-infrared photometry of 5 active main belt objects (AMBOs) detected by the Wide-field Infrared Survey Explorer (WISE) spacecraft. Four of these bodies, P/2010 R2 (La Sagra), 133P/Elst-Pizarro, (596) Scheila,…

We present a new analysis of ${\it Spitzer}$ observations of comet 29P/Schwassmann-Wachmann 1 taken on UT 2003 November 21, 23, and 24, similar to a previous investigation of the observations (Stansberry et al. 2004), but using the most…

Earth and Planetary Astrophysics · Physics 2015-08-06 Charles A. Schambeau , Yanga R. Fernandez , Carey M. Lisse , Nalin Samarasinha , Laura M. Woodney

We perform the first kinematic analysis of a CME observed by both imaging and in situ instruments on board STEREO, namely the SECCHI, PLASTIC, and IMPACT experiments. Launched on 2008 February 4, the CME is tracked continuously from…

Astrophysics · Physics 2011-02-11 B. E. Wood , R. A. Howard , S. P. Plunkett , D. G. Socker

We report results from new and archival observations of the newly discovered active asteroid (248370) 2005 QN_137, which has been determined to be a likely main-belt comet based on a subsequent discovery that it is recurrently active near…

I present the results of the first comprehensive effort aimed at modeling a major component of the stream of SOHO sungrazers, 5000 of which have been detected by the onboard coronagraphs since 1996. The stream of Population I of the Kreutz…

Earth and Planetary Astrophysics · Physics 2024-04-02 Zdenek Sekanina

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…

Earth and Planetary Astrophysics · Physics 2020-07-06 Quanzhi Ye , Tony L. Farnham , Matthew M. Knight , Carrie E. Holt , Lori M. Feaga

We present observations of comet 67P/Churyumov-Gerasimenko during its 2021/22 apparition, aiming to investigate its dust and gas environment and compare the results with those obtained in 2015/16 using the same telescope. Quasi-simultaneous…

Earth and Planetary Astrophysics · Physics 2025-09-17 V. Rosenbush , V. Kleshchonok , O. Ivanova , I. Luk'yanyk , C. Snodgrass , D. Gardener , L. Kolokolova , J. Markkanen , E. Shablovinskaya

Dormant or near-dormant short-period comets can unexpectedly regain ability to eject dust. In many known cases, the resurrection is short-lived and lasts less than one orbit. However, it is possible that some resurrected comets can remain…

Earth and Planetary Astrophysics · Physics 2017-04-19 Quan-Zhi Ye

The nearly continuous stream of miniature comets dominated by the Kreutz sungrazers has been an unexpected bonanza for cometary science initiated by the launch of the Solar and Heliospheric Observatory (SOHO) in 1995. Over the nearly 30…

Earth and Planetary Astrophysics · Physics 2024-01-04 Zdenek Sekanina

We present observations of main-belt comet 358P/PANSTARRS (P/2012 T1) obtained using the Gemini South telescope from 2017 July to 2017 December, as the object approached perihelion for the first time since its discovery. We find best-fit…

103P/Hartley 2 was selected as the target comet for the Deep Impact extended mission, EPOXI, in October 2007. There have been no direct optical observations of the nucleus of this comet, as it has always been highly active when previously…

Earth and Planetary Astrophysics · Physics 2015-05-18 Colin Snodgrass , Karen Meech , Olivier Hainaut
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