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相关论文: New Recurrently Active Main-belt Comet 2010 LH15

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Splitting of the nuclei of comets into multiple components has been frequently observed but, to date, no main-belt asteroid has been observed to break-up. Using the Hubble Space Telescope, we find that main-belt asteroid P/2013 R3 consists…

地球与行星天体物理 · 物理学 2015-06-19 David Jewitt , Jessica Agarwal , Jing Li , Harold Weaver , Max Mutchler , Stephen Larson

We present the results of our search for a dynamical family around the active asteroid P/2012F5 (Gibbs). By applying the hierarchical clustering method, we discover an extremely compact 9-body cluster associated with P/2012F5. The…

地球与行星天体物理 · 物理学 2014-01-14 Bojan Novakovic , Henry H. Hsieh , Alberto Cellino , Marco Micheli , Marco Pedani

During the planet formation process, billions of comets are created and ejected into interstellar space. The detection and characterization of such interstellar comets (also known as extra-solar planetesimals or extra-solar comets) would…

地球与行星天体物理 · 物理学 2016-07-28 Nathaniel V. Cook , Darin Ragozzine , Mikael Granvik , Denise C. Stephens

(modified from published version) Twelve years ago the Catalina Sky Survey discovered Earth's first known natural geocentric object other than the Moon, a few-meter diameter asteroid designated 2006 RH120. Despite significant improvements…

Jupiter-family comet 15P/Finlay has been reportedly quiet in activity for over a century but has harbored two outbursts during its 2014/2015 perihelion passage. Here we present an analysis of these two outbursts using a set of cometary…

地球与行星天体物理 · 物理学 2015-10-23 Quan-Zhi Ye , Peter G. Brown , Charles Bell , Xing Gao , Martin Mašek , Man-To Hui

We present a study of two newly discovered heliocentric hyperbolic objects -- 2017 U7 and 2018 C2. Both are possibly thermally evolved comets. Observations of the latter in 2018 March from Xingming Observatory revealed that it has a color…

地球与行星天体物理 · 物理学 2018-08-08 Man-To Hui

Eleven years after its perihelion, comet C/1995 O1 (Hale-Bopp) is still active. Between October 20--22, 2007, we detected a diffuse coma of 180x10^3$km in diameter with a slight elongation toward N/S direction. The integrated brightness was…

天体物理学 · 物理学 2009-11-13 Gy. M. Szabo , L. L. Kiss , K. Sarneczky

We present a physical characterization of main-belt comet 176P/LINEAR. Observations show the object exhibiting a fan-shaped tail in late 2005, but then becoming inactive in early 2006. Using data from 2007 when the object was observed to be…

地球与行星天体物理 · 物理学 2015-05-28 Henry H. Hsieh , Masateru Ishiguro , Pedro Lacerda , David Jewitt

The unique inner-belt asteroid 311P/PANSTARRS (formerly P/2013 P5) is notable for its sporadic, comet-like ejection of dust in nine distinct epochs spread over $\sim$250 days in 2013. This curious behavior has been interpreted as the…

地球与行星天体物理 · 物理学 2018-05-23 David Jewitt , Harold Weaver , Max Mutchler , Jing Li , Jessica Agarwal , Stephen Larson

We present VRI spectrophotometry of 1003 Main-Belt Asteroids (MBAs) observed with the Sutherland, South Africa, node of the Korea Microlensing Telescope Network (KMTNet). All of the observed MBAs were serendipitously captured in KMTNet's…

地球与行星天体物理 · 物理学 2018-08-01 N. Erasmus , A. McNeill , M. Mommert , D. E. Trilling , A. A. Sickafoose , C. van Gend

Studying materials released from Jupiter-family comets (JFCs) -- as seen in their inner com\ae, the envelope of gas and dust that forms as the comet approaches the Sun -- improves the understanding of their origin and evolutionary history.…

We present archival observations demonstrating that main belt asteroid (6478) Gault has an extensive history of comet-like activity. Outbursts have taken place during multiple epochs since 2013 and at distances extending as far as 2.68 au,…

地球与行星天体物理 · 物理学 2019-05-03 Colin Orion Chandler , Jay Kueny , Annika Gustafsson , Chadwick A. Trujillo , Tyler D. Robinson , David E. Trilling

We describe active asteroid 331P/Gibbs (2012 F5) using archival Hubble Space Telescope data taken between 2015 and 2018. 331P is an outer main-belt active asteroid with a long-lived debris trail that formed in 2011. Embedded in the debris…

地球与行星天体物理 · 物理学 2021-12-08 David Jewitt , Jing Li , Yoonyoung Kim

The tremendous tidal force that is linked to the supermassive black hole (SMBH) at the center of our galaxy is expected to strongly subdue star formation in its vicinity. Stars within 1" from the SMBH thus likely formed further from the…

Stellar-mass black holes (BHs), with masses comparable to stars, are a major constituent of our Milky Way galaxy. This chapter describes the landscape of challenging, and long-sought efforts to identify these objects in the Galaxy. The…

高能天体物理现象 · 物理学 2023-04-20 Morgan MacLeod , Jonathan Grindlay

1I/2017 U1 (`Oumuamua), a recently discovered asteroid in a hyperbolic orbit, is likely the first macroscopic object of extrasolar origin identified in the solar system. Here, we present imaging and spectroscopic observations of…

地球与行星天体物理 · 物理学 2017-12-20 Quan-Zhi Ye , Qicheng Zhang , Michael S. P. Kelley , Peter G. Brown

We present the physical and dynamical properties of the recently discovered active asteroid (248370) 2005 QN173 (aka 433P). From our observations, we derived two possible rotation period solutions of 2.7 and 4.1 hours. The corresponding…

地球与行星天体物理 · 物理学 2022-09-05 Bojan Novakovic , Debora Pavela , Henry H. Hsieh , Dusan Marceta

We present Hubble Space Telescope Observations of (596) Scheila during its recent dust outburst. The nucleus remained point-like with absolute magnitude V(1,1,0) = 8.85+/-0.02 in our data, equal to the pre-outburst value, with no secondary…

地球与行星天体物理 · 物理学 2015-05-27 David Jewitt , Harold Weaver , Max Mutchler , Stephen Larson , Jessica Agarwal

The quest for quiet or dormant black holes has been ongoing since several decades. Ellipsoidal variables possibly indicate the existence of a very high-mass invisible companion and are thought to be one of the best ways to find such dormant…

The quasi-Hilda object, 212P/2000YN30 with a cometary-like orbit, was found to display a dust tail structure between January and March, 2009. From orbital calculations, it is shown that this object could have been an active comet in its…

太阳与恒星天体物理 · 物理学 2015-06-15 Y. -C. Cheng , W. -H. Ip