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We present OSIRIS/NAC observations of decimetre-sized, likely ice-containing aggregates ejected from a confined region on the surface of comet 67P/Churyumov-Gerasimenko. The images were obtained in January 2016 when the comet was at 2 AU…

We report photometry of three outbursts of NN Cam in 2007, 2008 and 2009. The 2007 event started with a normal outburst, lasting about 4 days, which was a precursor to a superoutburst lasting at least 13 days. Both the precursor and the…

The release of volatiles from comets is usually from direct sublimation of ices on the nucleus, but for very or hyper-active comets other sources have to be considered to account for the total production rates. In this work, we present new…

地球与行星天体物理 · 物理学 2023-04-13 Theodore Kareta , John W. Noonan , Walter M. Harris , Alessondra Springmann

During its two years mission around comet 67P/Churyumov-Gerasimenko, ESA's Rosetta spacecraft had the unique opportunity to follow closely a comet in the most active part of its orbit. Many studies have presented the typical features…

We report on time-resolved photometry of the 2005 July superoutburst of the dwarf nova, 2QZ J021927.9-304545. The resultant light curves showed conspicuous superhumps with a period of 0.081113(19) days, confirming the SU UMa nature of the…

天体物理学 · 物理学 2015-06-24 Akira Imada , Taichi Kato , L. A. G. Monard , Alon Retter , Alex Liu , Daisaku Nogami

Alice is a far-ultraviolet imaging spectrograph onboard Rosetta that, amongst multiple objectives, is designed to observe emissions from various atomic and molecular species from within the coma of comet 67P/Churyumov-Gerasimenko. The…

We discuss the morphology and spectrophotometry of 5 comets visible in August, 2001. We decompose comae into coma profiles and azimuthally renormalized images, in which general and local features are quantitatively comparable. Comet…

天体物理学 · 物理学 2009-11-07 Gy. M. Szabo , L. L. Kiss , K. Sarneczky , K. Sziladi

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.…

Comet 7P/Pons-Winnecke was observed from the Calar Alto Observatory (Spain) for four months during the 2021 inbound apparition. Broad-band visible images were taken between 1.71 and 1.25 AU pre-perihelion, while long-slit spectrophotometric…

地球与行星天体物理 · 物理学 2025-03-18 Irene Mariblanca-Escalona , Luisa M. Lara , Fernando Moreno , Pedro J. Gutiérrez , Marçal Evangelista-Santana

The Centaurs are the small solar system bodies intermediate between the active inner solar system Jupiter Family Comets and their inactive progenitors in the trans-Neptunian region. Among the fraction of Centaurs which show comet-like…

地球与行星天体物理 · 物理学 2020-01-08 Theodore Kareta , Benjamin Sharkey , John Noonan , Kathryn Volk , Vishnu Reddy , Walter Harris , Richard Miles

We report on the Hubble Space Telescope program to observe periodic comet 9P/Tempel 1 in conjunction with NASA's Deep Impact mission. Our objectives were to study the generation and evolution of the coma resulting from the impact and to…

The extraordinary 2021 September-October outburst of Centaur 29P/Schwassmann-Wachmann 1 afforded an opportunity to test the composition of primitive Kuiper disk material at high sensitivity. We conducted nearly simultaneous multi-wavelength…

We report CCD photometry and analysis of the first observed superoutburst of the SU UMa-type dwarf nova KP Cassiopeiae during 2008 October. We observed a distinct shortening of the superhump period at superhump cycle 15. Before that point…

太阳与恒星天体物理 · 物理学 2010-01-28 David Boyd , Pierre dePonthiere , Jerry Foote , Mack Julian , Taichi Kato , Robert Koff , Tom Krajci , Gary Poyner , Jeremy Shears , Bart Staels

The Rosetta space probe accompanied comet 67P/Churyumov-Gerasimenko for more than two years, obtaining an unprecedented amount of unique data of the comet nucleus and inner coma. This work focuses identifying the source regions of faint…

We present photometric observations of the dwarf nova 1RXS J053234.9+624755. We performed a detailed analysis of the superoutburst that occurred in August 2009. We found the superhump period to be P_sh=0.057122(14)days. Based on the O-C…

太阳与恒星天体物理 · 物理学 2011-01-06 A. Rutkowski , A. Olech , R. Poleski , M. Sobolewska , P. Kankiewicz , T. Ak , D. Boyd

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 observed the 1998 November superoutburst of WX Cet, a dwarf nova originally proposed as a WZ Sge-like system. The observation established that WX Cet is an SU UMa-type dwarf nova with a mean superhump period of 0.05949(1) d, which is…

天体物理学 · 物理学 2015-06-24 Taichi Kato , Katsura Matsumoto , Daisaku Nogami , Koichi Morikawa , Seiichiro Kiyota

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…

地球与行星天体物理 · 物理学 2025-09-17 V. Rosenbush , V. Kleshchonok , O. Ivanova , I. Luk'yanyk , C. Snodgrass , D. Gardener , L. Kolokolova , J. Markkanen , E. Shablovinskaya

We observed the split comet 157P/Tritton in October - November 2022 and January 2024 with the Nordic Optical Telescope (NOT). Our observations show that the splitting continued during the entire observing campaign. Fragmentation was…

地球与行星天体物理 · 物理学 2025-01-07 Jane Luu , David Jewitt

We report photometric observations of AL Com during its rare outburst in 2007. The light curve is reminiscent of its past superoutbursts in 1995 and 2001, except for the rebrightening phase after the main superoutburst. During the…

天体物理学 · 物理学 2008-02-01 M. Uemura , A. Arai , M. Sasada , P. Schmeer , I. Miller , T. Ohsugi , T. Yamashita , K. S. Kawabata , M. Isogai , S. Sato , M. Kino