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相关论文: The Yarkovsky and YORP Effects

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Five new correlations between sunspot activity and orbiting position of the Jovian planets are detected. In order to explain these correlations it is suggested that the resonance of the outer planets destabilizes the orbit of Kuiper Belt…

综合物理 · 物理学 2009-06-25 Jozsef Garai

Gravitational and electronic forces produce a correlation between the mass and shape of objects in the universe. For example, at an average radius of ~ 200 km - 300 km, the icy moons and rocky asteroids of our Solar System transition from a…

地球与行星天体物理 · 物理学 2010-04-08 Charles H. Lineweaver , Marc Norman

The terrestrial planets formed by accretion of asteroid-like objects within the inner solar system's protoplanetary disk. Previous works have found that forming a small-mass Mars requires the disk to contain little mass beyond ~1.5 au…

地球与行星天体物理 · 物理学 2023-06-16 Patryk Sofia Lykawka , Takashi Ito

Spin state predictions for defunct satellites in geosynchronous earth orbit (GEO) are valuable for active debris removal and servicing missions as well as material shedding studies and attitude-dependent solar radiation pressure (SRP)…

地球与行星天体物理 · 物理学 2022-10-31 Conor J. Benson , Daniel J. Scheeres

(abbreviated) We extend the theory of close encounters of a planet on a parabolic orbit with a star to include the effects of tides induced on the central rotating star. Orbits with arbitrary inclination to the stellar rotation axis are…

地球与行星天体物理 · 物理学 2015-05-28 P. B. Ivanov , J. C. B. Papaloizou

Out of nine known stable Mars Trojans, seven appear to be members of an orbital grouping including the largest Trojan, Eureka. In order to test if this could be a genetic family, we simulated the long term evolution of a tight orbital…

地球与行星天体物理 · 物理学 2015-06-23 Matija Ćuk , Apostolos A. Christou , Douglas P. Hamilton

Asteroid families are formed as the result of collisions. Large fragments are ejected with speeds of the order of the escape velocity from the parent body. After the family formation, the fragments' orbits evolve in the space of proper…

地球与行星天体物理 · 物理学 2018-04-03 V. Carruba , D. Vokrouhlický , B. Novakovic

The inner asteroid belt between 2.1 and 2.5 au is of particular dynamical significance because it is the dominant source of both chondritic meteorites and near-Earth asteroids. This inner belt is bounded by an eccentricity-type secular…

地球与行星天体物理 · 物理学 2022-09-14 Apostolos A. Christou , Stanley F. Dermott , Dan Li

The origin of rings around giant planets remains elusive. Saturn's rings are massive and made of 90-95% of water ice. In contrast, the much less massive rings of Uranus and Neptune are dark and likely to have higher rock fraction. Here we…

地球与行星天体物理 · 物理学 2016-11-15 Ryuki Hyodo , Sébastien Charnoz , Keiji Ohtsuki , Hidenori Genda

Many asteroids in the main belt are continuously pushed by Yarkovsky effect into regions of different mean motion resonances (MMRs) and then ejected out. They are considered as the principal source of near-Earth objects. We investigate in…

地球与行星天体物理 · 物理学 2020-05-06 Yang-Bo Xu , Li-Yong Zhou , Wing-Huen Ip

The primary objective of this study was to utilize the newest Gaia FPR catalogue containing ultra-precise asteroid astrometry spanning over 66 months to detect the Yarkovsky effect, a non-gravitational acceleration that affects the orbits…

地球与行星天体物理 · 物理学 2024-12-25 Karolina Dziadura , Przemysław Bartczak , Dagmara Oszkiewicz

Video observations of Jupiter obtained by amateur astronomers over the past eight years have shown five flashes of light of 1-2 s. The first three of these events occurred on 3 June 2010, 20 August 2010, and 10 September 2012. Previous…

Through the Rossiter-McLaughlin effect, several hot Jupiters have been found to exhibit spin-orbit misalignment, and even retrograde orbits. The high obliquity observed in these planets can be attributed to two primary formation mechanisms,…

地球与行星天体物理 · 物理学 2025-01-13 Huan-rong Yuan , Ying Wang , Xin Wu , Ji-wei Xie , Hui-gen Liu , Ji-lin Zhou , Wei Sun

We consider a special relativistic effect, known as the Poynting-Robertson effect, on various types of trajectories of solar sails. Since this effect occurs at order $v^{\phi}/c$, where $v^{\phi}$ is the tangential speed relative to the…

空间物理 · 物理学 2010-12-17 Roman Ya. Kezerashvili , Justin F. Vazquez-Poritz

Giant planets orbiting main-sequence stars closer than 0.1 AU are called hot Jupiters. They interact with their stars affecting their angular momentum. Recent observations provide suggestive evidence of excess angular momentum in stars with…

太阳与恒星天体物理 · 物理学 2015-05-14 A. F. Lanza

A relativistic electron uniformly rotating along a shifted equatorial orbit about a dielectric ball may generate microwave Cherenkov radiation tens of times more intense as that generated at the revolution in a continuous, infinite and…

经典物理 · 物理学 2010-07-19 L. Sh. Grigoryan , H. F. Khachatryan , S. R. Arzumanyan , M. L. Grigoryan

A star in the Milky Way's disk can now be at a Galactocentric radius quite distant from its birth radius for two reasons: either its orbit has become eccentric through radial heating, which increases its radial action $J_R$ (`blurring'); or…

星系天体物理 · 物理学 2020-06-17 Neige Frankel , Jason Sanders , Yuan-Sen Ting , Hans-Walter Rix

Rotation period clustering in prograde/retrograde rotators might indicate the preliminary indication of the Slivan state in the Koronis family as a result of the YORP effect. We follow the general scenario of dispersion in semimajor axis of…

地球与行星天体物理 · 物理学 2016-01-14 Chan-Kao Chang , Hsing-Wen Lin , Wing-Huen Ip

Anisotropic outgassing from comets exerts a torque sufficient to rapidly change the angular momentum of the nucleus, potentially leading to rotational instability. Here, we use empirical measures of spin changes in a sample of comets to…

地球与行星天体物理 · 物理学 2021-05-19 David Jewitt

The Sun was an order of magnitude more luminous during the first few hundred thousand years of its existence, due in part to the gravitational energy released by material accreting from the Solar nebula. If Jupiter was already near its…

地球与行星天体物理 · 物理学 2015-05-30 N. J. Turner , M. Choukroun , J. Castillo-Rogez , G. Bryden