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We aim to characterize the physical and activity properties of the interstellar comet 3I/ATLAS through spectroscopic and photometric observations during the first month after its discovery. We performed time-series photometry and long-slit…

地球与行星天体物理 · 物理学 2025-10-01 T. Santana-Ros , O. Ivanova , S. Mykhailova , N. Erasmus , K. Kamiński , D. Oszkiewicz , T. Kwiatkowski , M. Husárik , T. S. Ngwane , A. Penttilä

Main belt asteroid (6478) Gault has been dynamically linked with two overlapping asteroid families: Phocaea, dominated by S-type asteroids, and Tamara, dominated by low-albedo C-types. This object has recently become an interesting case for…

地球与行星天体物理 · 物理学 2019-08-14 Juan A. Sanchez , Vishnu Reddy , Audrey Thirouin , Edward L. Wright , Tyler R. Linder , Theodore Kareta , Benjamin Sharkey

At discovery time, C/2017 K2 (PANSTARRS) was the second most distant inbound active comet ever observed. It has been argued that this object is in the process of crossing the inner Solar System for the first time, but other authors have…

地球与行星天体物理 · 物理学 2018-04-25 R. de la Fuente Marcos , C. de la Fuente Marcos

A new asteroid rotation period survey have been carried out by using the Palomar Transient Factory (PTF). Twelve consecutive PTF fields, which covered an area of 87 deg$^2$ in the ecliptic plane, were observed in $R$ band with a cadence of…

We revisited a mass ejection phenomenon that occurred in asteroid P/2010 A2 in terms of the dynamical properties of the dust particles and large fragments. We constructed a model assuming anisotropic ejection within a solid cone-shaped jet…

地球与行星天体物理 · 物理学 2017-05-03 Yoonyoung Kim , Masateru Ishiguro , Tatsuhiro Michikami , Akiko M. Nakamura

Comet C/2025 K1 (ATLAS) reached perihelion at 0.33 au on 2025 October 8. Daily monitoring by the LCO Outbursting Objects Key Project revealed a major activity increase between November 2 and 4, accompanied by rapid changes in coma…

We present new optical coronagraphic data of the bright star Fomalhaut obtained with the HST in 2010/2012 using STIS. Fomalhaut b is recovered at both epochs to high significance. The observations include the discoveries of tenuous…

地球与行星天体物理 · 物理学 2015-06-15 Paul Kalas , James R. Graham , Michael P. Fitzgerald , Mark Clampin

Distant long-period comet C/2017 K2 has been outside the planetary region of the solar system for 3 Myr, negating the possibility that heat retained from the previous perihelion could be responsible for its activity. This inbound comet is…

地球与行星天体物理 · 物理学 2019-01-30 David Jewitt , Jessica Agarwal , Man-To Hui , Jing Li , Max Mutchler , Harold Weaver

A class of asteroids, called large super-fast rotators (large SFRs), have rotation periods shorter than 2 hours and diameters larger than ~ 0.3 km. They pose challenges to the usual interior rubble-pile structure unless a relatively high…

We present a study of interstellar comet 2I/2019 Q4 (Borisov) using both preperihelion and postperihelion observations spanning late September 2019 through late January 2020. The intrinsic brightness of the comet was observed to…

地球与行星天体物理 · 物理学 2020-06-17 Man-To Hui , Quan-Zhi Ye , Dora Föhring , Denise Hung , David J. Tholen

We report the observations of solar system objects during the 2015 campaign of the High cadence Transient Survey (HiTS). We found 5740 bodies (mostly Main Belt asteroids), 1203 of which were detected in different nights and in $g'$ and…

We present ALMA observations of the CO(2-1) and CO(3-2) molecular gas transitions and associated (sub)-mm continua of the nearby Seyfert 1.5 galaxy NGC3227 with angular resolutions 0.085-0.21" (7-15pc). On large scales the cold molecular…

It has been suggested that the comet-like activity of Main Belt Comets is due to the sublimation of sub-surface water-ice that is exposed when these objects are impacted by meter-sized bodies. We recently examined this scenario and showed…

地球与行星天体物理 · 物理学 2018-03-21 Nader Haghighipour , Thomas I. Maindl , Christoph M. Schaefer , Oliver J. Wandel

Comet C/2016 R2 (PanSTARRS) has a peculiar volatile composition, with CO being the dominant volatile as opposed to H$_2$O and one of the largest N$_2$/CO ratios ever observed in a comet. Using observations obtained with the \textit{Spitzer…

C/2002 CE$_{10}$ is an object in a retrograde elliptical orbit with Tisserand parameter $-0.853$ indicating a likely origin in the Oort Cloud. It appears to be a rather inactive comet since no coma and only a very weak tail was detected…

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…

地球与行星天体物理 · 物理学 2015-08-06 Charles A. Schambeau , Yanga R. Fernandez , Carey M. Lisse , Nalin Samarasinha , Laura M. Woodney

Ejection of large boulder-like debris is a vigorous form of cometary activity that is unlikely induced by water ice out-gassing alone but rather associated with the sublimation of super-volatile ices. Though perceived on several comets,…

地球与行星天体物理 · 物理学 2024-01-31 Xian Shi , Xuanyu Hu , Jessica Agarwal , Carsten Güttler , Martin Rose , Horst Uwe Keller , Marco Fulle , Jakob Deller , Holger Sierks

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

The asteroids are primitive solar system bodies which evolve both collisionally and through disruptions due to rapid rotation [1]. These processes can lead to the formation of binary asteroids [2-4] and to the release of dust [5], both…

地球与行星天体物理 · 物理学 2017-10-11 Jessica Agarwal , David Jewitt , Max Mutchler , Harold Weaver , Stephen Larson

We have used the infrared mineralogical model derived from the Spitzer IRS observations of the Deep Impact experiment to study the nature of the dust in the debris found around the K0V star HD69830 (Beichman et al. 2005). Using a robust…

天体物理学 · 物理学 2009-01-19 C. M. Lisse , C. A. Beichman , G. Bryden , M. C. Wyatt
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