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相关论文: Bi-lobed Shape of Comet 67P from a Collapsed Binar…

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On January 18-19 and June 28-29 of 2010, the Wide-field Infrared Survey Explorer (WISE) spacecraft imaged the Rosetta mission target, comet 67P/Churyumov-Gerasimenko. We present a preliminary analysis of the images, which provide a…

As indicated by their special characteristics, the cold classical Kuiper belt objects (KBOs) formed and survived at 42-47 au. Notably, they show a large fraction of equal-size binaries whose formation is probably related to the accretion of…

地球与行星天体物理 · 物理学 2019-05-29 David Nesvorny , David Vokrouhlicky

The binary asteroid 288P/(300163) is unusual both for its combination of wide-separation and high mass ratio and for its comet-like activity. It is not currently known whether there is a causal connection between the activity and the…

地球与行星天体物理 · 物理学 2020-11-25 Jessica Agarwal , Yoonyoung Kim , David Jewitt , Max Mutchler , Harold Weaver , Stephen Larson

Short-period comet 108P/Ciffreo is known for its peculiar double morphology, in which the nucleus is accompanied by a co-moving, detached, diffuse 'blob'. We report new observations of 108P/Ciffreo taken with the Hubble Space Telescope and…

地球与行星天体物理 · 物理学 2023-03-15 Yoonyoung Kim , David Jewitt , Jane Luu , Jing Li , Max Mutchler

We report on the first major temporal morphological changes observed on the surface of the nucleus of comet 67P/Churyumov-Gerasimenko, in the smooth terrains of the Imhotep region. We use images of the OSIRIS cameras onboard Rosetta to…

Spin--orbit misalignment in coalescing compact binaries affects their gravitational radiation waveforms. When the misalignment angles are large (>30 degrees), the detection efficiency of the coalescence events can decrease significantly if…

天体物理学 · 物理学 2009-10-31 Vassiliki Kalogera

We present infrared images and spectra of comets 2P/Encke, 67P/Churyumov-Gerasimenko, and C/2001 HT50 (LINEAR-NEAT) as part of a larger program to observe comets inside of 5 AU from the sun with the Spitzer Space Telescope. The nucleus of…

Here we review some of the major findings of the mass spectrometer suite ROSINA on board of ESA's Rosetta spacecraft to comet 67P/Churyumov-Gerasimenko. For more than 2 years, ROSINA continuously measured the composition of the gases…

地球与行星天体物理 · 物理学 2023-09-15 Martin Rubin

The coma of comet 67P/Churyumov-Gerasimenko has been probed by the Rosetta spacecraft and shows a variety of different molecules. The ROSINA COmet Pressure Sensor and the Double Focusing Mass Spectrometer provide in-situ densities for many…

地球与行星天体物理 · 物理学 2022-02-11 Matthias Laeuter , Tobias Kramer , Martin Rubin , Kathrin Altwegg

Over 30 planetary systems have been discovered to reside in binary stars. For small separations gravitational perturbation of the secondary star has a strong influence on the planet formation process. It truncates the protoplanetary disk,…

天体物理学 · 物理学 2009-11-13 Wilhelm Kley , Richard Nelson

Methods. We algorithmically tracked thousands of individual particles through four OSIRIS/NAC image sequences of 67P's near-nucleus coma. We then traced concentrated particle groups back to the nucleus surface, and estimated their potential…

地球与行星天体物理 · 物理学 2024-05-22 Marius Pfeifer , Jessica Agarwal , Raphael Marschall , Björn Grieger , Pablo Lemos

Binaries occur in many astrophysical systems, from young protostellar binaries in star forming regions to supermassive black hole binaries in galaxy centers. In many cases, a circumbinary disk of gas forms around the binary with an orbit…

地球与行星天体物理 · 物理学 2026-01-12 Cheng Chen , Philip J. Armitage , C. J. Nixon

The conventional wisdom for the formation of the first hard binary in core collapse is that three-body interactions of single stars form many soft binaries, most of which are quickly destroyed, but eventually one of them survives. We report…

星系天体物理 · 物理学 2015-05-28 Ataru Tanikawa , Piet Hut , Junichiro Makino

We consider essential mechanisms for orbit-shrinkage or "hardening" of compact binaries in globular clusters to the point of Roche-lobe contact and X-ray emission phase, focussing on the process of collisional hardening due to encounters…

天体物理学 · 物理学 2009-11-11 S. Banerjee , P. Ghosh

The Rosetta mission provided us with detailed data of the surface of the nucleus of comet 67P/Churyumov-Gerasimenko.In order to better understand the physical processes associated with the comet activity and the surface evolution of its…

地球与行星天体物理 · 物理学 2021-05-26 A. Bouquety , L. Jorda , O. Groussin , A. Sejourné , S. Bouley , F. Costard

I list the 16 planetary nebulae (PNe) known to contain close-binary nuclei, and show that the nebulae generally have axisymmetric structures, including elliptical, bipolar, or ring morphologies. The orbital periods range from 2.7 hr to 16…

天体物理学 · 物理学 2007-05-23 Howard E. Bond

The cometary materials are thought to be the reservoir of primitive materials in the Solar System. The recent detection of glycine and CH$_3$NH$_2$ by the ROSINA mass spectrometer in the coma of 67P/Churyumov-Gerasimenko suggests that amino…

地球与行星天体物理 · 物理学 2021-02-03 Taiki Suzuki , Yoshiharu Shinnaka , Liton Majumdar , Takashi Shibata , Yuhito Shibaike , Hideko Nomura , Harumi Minamoto

Previous high resolution cosmological simulations predict the first stars to appear in the early universe to be very massive and to form in isolation. Here we discuss a cosmological simulation in which the central 50 solar mass clump breaks…

宇宙学与河外天体物理 · 物理学 2009-07-20 Matthew J. Turk , Tom Abel , Brian W. O'Shea

With the discovery of Kuiper Belt binaries that have wide separations and roughly equal masses new theories were proposed to explain their formation. Two formation scenarios were suggested by Goldreich and collaborators: In the first,…

天体物理学 · 物理学 2009-11-13 Hilke E. Schlichting , Re'em Sari

The data obtained in the recent Rosetta space mission to comet 67P/Churyumov-Gerasimenko have had a profound impact on the understanding of the nature of comets. In addition to revising the notions on the physical properties and structure…

地球与行星天体物理 · 物理学 2019-12-24 V. V. Emel'yanenko