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相关论文: Oort spike comets with large perihelion distances

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The second Gaia data release (Gaia DR2) provided us with the precise five-parameter astrometry for 1.3 billion of sources. As stars passing close to the Solar System are thought to be responsible for influencing the dynamical history of…

地球与行星天体物理 · 物理学 2022-01-31 Rita Wysoczańska , Piotr A. Dybczyński , Magdalena Polińska

The interstellar comet 2I/Borisov bears a strong resemblance to Oort Cloud comets, judging from its appearance in images taken over the first six weeks of observation. To test the proposed affinity in more diagnostic terms, 2I is compared…

地球与行星天体物理 · 物理学 2019-10-23 Zdenek Sekanina

The star $\beta$ Pictoris harbors a young planetary system, which is characterized by the presence of a gaseous and dusty debris disk, at least two massive planets and many minor bodies. For more than thirty years, exocomets transiting the…

A group of newly observed extreme trans-Neptunian objects exhibit unexpected orbital confinement, characterized by the alignment of orbital angular momentum vectors and apsidal lines. It is proposed that an undiscovered giant planet, named…

地球与行星天体物理 · 物理学 2025-01-29 Rafael Ribeiro , Andre Izidoro , Alessandro Morbidelli , David Nesvorny , Othon Cabo Winter

Small bodies are capable of delivering essential prerequisites for the development of life, such as volatiles and organics, to the terrestrial planets. For example, empirical evidence suggests that water was delivered to the Earth by…

We examine the orbital element distribution of main-belt comets (MBCs), which are objects that exhibit cometary activity yet orbit in the main asteroid belt, and may be potentially useful as tracers of ice in the inner solar system. We find…

地球与行星天体物理 · 物理学 2018-03-21 Yoonyoung Kim , Youngmin JeongAhn , Henry H. Hsieh

(Abridged) The solar system gas giant planets are oblate due to their rapid rotation. A measurement of the planet's projected oblateness would constrain the planet's rotational period. Planets that are synchronously rotating with their…

天体物理学 · 物理学 2009-11-07 S. Seager , Lam Hui

The dynamics of small bodies perturbed by an eccentric planet was done mostly under the assumption of well separated orbits using analytical approximations appropriate for the hierarchical case. In this work we study the dynamics of small…

地球与行星天体物理 · 物理学 2025-07-28 Tabare Gallardo , Rodrigo Cabral

In the framework of the emergent gravity scenario by Verlinde, it was recently observed by Liu and Prokopec that, among other things, an anomalous pericenter precession would affect the orbital motion of a test particle orbiting an isolated…

广义相对论与量子宇宙学 · 物理学 2017-03-14 Lorenzo Iorio

The Mars flyby of C/2013 A1 (Siding Spring) represented a unique opportunity for imaging a long-period comet and resolving its nucleus and rotation period. Because of the small encounter distance and the high relative velocity, the goal of…

地球与行星天体物理 · 物理学 2016-05-04 D. Farnocchia , S. R. Chesley , M. Micheli , A. Delamere , R. S. Heyd , D. J. Tholen , J. D. Giorgini , W. M. Owen , L. K. Tamppari

Aims. Investigate the influence of cluster environments on asteroids, with special attention towards captured material. Methods. Using numerical methods, a sub-virial fractally distributed star-forming region and a virialised Plummer…

地球与行星天体物理 · 物理学 2026-05-29 Erwan Hochart , Simon Portegies Zwart

On 2018 November 18, coronagraphs onboard the Solar and Heliospheric Observatory (SOHO) captured an unrecognized comet crossing its fields of view. We identified this comet to be the minor planet (139359) 2001 ME1 whose previously unnoticed…

地球与行星天体物理 · 物理学 2026-02-09 Qicheng Zhang , Quanzhi Ye , Karl Battams , Matthew M. Knight , Worachate Boonplod , Rainer Kracht

Passing stars may play an important role in the evolution of our solar system. We search for close stellar encounters to the Sun among all 7.2 million stars in Gaia-DR2 that have six-dimensional phase space data. We characterize encounters…

太阳与恒星天体物理 · 物理学 2018-08-15 C. A. L. Bailer-Jones , J. Rybizki , R. Andrae , M. Fouesneau

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…

Around low- and intermediate-mass (1.5-3 M_sun) red giants, no planets have been found inside 0.6 AU. Such a paucity is not seen in the case of 1 M_sun main sequence stars. In this study, we examine the possibility that short-period planets…

地球与行星天体物理 · 物理学 2015-05-27 M. Kunitomo , M. Ikoma , B. Sato , Y. Katsuta , S. Ida

Motivated by recent data on comets in the low corona, we discuss destruction of sun impacting comets in the dense lower solar atmosphere. Perihelion distances q less than the solar radius and incident masses Mo much greater than 1E12 g are…

太阳与恒星天体物理 · 物理学 2015-07-22 John C. Brown , Robert W. Carlson , Mark P. Toner

We present numerical simulations to model the production of observable long-period comets (LPCs) from the Oort Cloud, a vast reservoir of icy bodies surrounding the Sun. We show that inner Oort Cloud objects can penetrate Jupiter's orbit…

地球与行星天体物理 · 物理学 2014-11-20 Nathan A. Kaib , Thomas Quinn

A sequence of events, dominated by two outbursts and ending with the preperihelion disintegration of comet C/2017 S3, is examined. The onset times of the outbursts are determined with high accuracy from the light curve of the nuclear…

地球与行星天体物理 · 物理学 2019-01-30 Zdenek Sekanina , Rainer Kracht

The practical distinctions between asteroids and comets, viewed as products of accretion on either side of the snow line, are less clear-cut than previously understood. In this chapter, we discuss the numerous solar system populations which…

地球与行星天体物理 · 物理学 2022-12-06 David Jewitt , Henry H. Hsieh

We report the first results of a research program to explore the sensitivity of the orbits of Oort cloud comets to changes in the strength of the Galactic tides in the plane of the disk and also to changes in the mass of the host star. We…

星系天体物理 · 物理学 2014-11-20 Marco Masi , Luigi Secco , Guillermo Gonzalez
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