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Dormant comets in the near-Earth object (NEO) population are thought to be involved in the terrestrial accretion of water and organic materials. Identification of dormant comets is difficult as they are observationally indistinguishable…

Earth and Planetary Astrophysics · Physics 2016-09-07 Quan-Zhi Ye , Peter G. Brown , Petr Pokorný

Context. Asteroids with semi-major axes very close to that of a host planet can avoid node crossings when their nodal points are at perihelion and at aphelion. This layout protects the asteroids from close encounters, and eventual…

Earth and Planetary Astrophysics · Physics 2015-08-19 C. de la Fuente Marcos , R. de la Fuente Marcos

Recent dynamical analyses suggest that some Jupiter family comets (JFCs) may originate in the main asteroid belt instead of the outer solar system. This possibility is particularly interesting given evidence that icy main-belt objects are…

Earth and Planetary Astrophysics · Physics 2020-04-08 Henry H. Hsieh , Bojan Novakovic , Kevin J. Walsh , Norbert Schorghofer

Earth co-orbitals of the horseshoe type are interesting objects to study for practical reasons. They are relatively easy to access from our planet and that makes them attractive targets for sample return missions. Here, we show that…

Earth and Planetary Astrophysics · Physics 2015-12-14 C. de la Fuente Marcos , R. de la Fuente Marcos

It is commonly accepted that quasar redshifts have a cosmological character and that most of the quasars are at Gigaparsec distances. However, there are some cases where several quasars with completely different redshifts and a nearby…

Astrophysics · Physics 2009-11-10 Piotr Popowski , Wolfgang Weinzierl

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…

Earth and Planetary Astrophysics · Physics 2022-09-05 Bojan Novakovic , Debora Pavela , Henry H. Hsieh , Dusan Marceta

Context. Jupiter-family comets (JFCs), which originate from the Kuiper belt and scattered disk, exhibit low-inclination and chaotic trajectories due to close encounters with Jupiter. Despite their typically short incursions into the inner…

Earth and Planetary Astrophysics · Physics 2024-10-01 P. M. Shober , G. Tancredi , J. Vaubaillon , H. A. R. Devillepoix , S. Deam , S. Anghel , E. K. Sansom , F. Colas , S. Martino

The orbital evolution of about 20000 Jupiter-crossing objects and 1500 resonant asteroids under the gravitational influence of planets was investigated. The rate of their collisions with the terrestrial planets was estimated by computing…

Astrophysics · Physics 2010-12-01 S. I. Ipatov , J. C. Mather

Jupiter-family Comet D/1770 L1 (Lexell) was the first discovered Near-Earth Object (NEO), and passed the Earth on 1770 Jul 1 at a recorded distance of 0.015 au. The comet was subsequently lost due to unfavorable observing circumstances…

Earth and Planetary Astrophysics · Physics 2018-04-04 Quan-Zhi Ye , Paul A. Wiegert , Man-To Hui

Centaurs--icy bodies orbiting beyond Jupiter and interior to Neptune--are believed to be dynamically related to Jupiter Family Comets (JFCs), which have aphelia near Jupiter's orbit and perihelia in the inner Solar System. Previous…

Earth and Planetary Astrophysics · Physics 2019-10-23 Kevin R. Grazier , Jonathan Horner , Julie C. Castillo-Rogez

The organization of the orbits of most minor bodies in the Solar system seems to follow random patterns, the result of billions of years of chaotic dynamical evolution. Much as heterogeneous orbital behaviour is ubiquitous, dynamically…

Earth and Planetary Astrophysics · Physics 2017-12-08 C. de la Fuente Marcos , R. de la Fuente Marcos

Most co-orbital objects in the Solar system are thought to follow tadpole-type orbits, behaving as Trojans. However, most of Earth's identified co-orbitals are moving along horseshoe-type orbits. The current tally of minor bodies considered…

Earth and Planetary Astrophysics · Physics 2020-07-08 Murat Kaplan , Sergen Cengiz

The Centaurs are recent escapees from the Kuiper belt that are destined either to meet fiery oblivion in the hot inner regions of the Solar system or to be ejected to the interstellar medium by gravitational scattering from the giant…

Earth and Planetary Astrophysics · Physics 2009-11-13 David Jewitt

Context. Natural interstellar objects do not form isolated in deep space, but escape their natal planetary systems. Early removal from their home star systems via close flybys with still-forming planets could be the dominant ejection…

Earth and Planetary Astrophysics · Physics 2024-10-25 R. de la Fuente Marcos , C. de la Fuente Marcos , S. J. Aarseth

We provide context for Apophis' 2029 Earth passage by analyzing its possible source populations, in particular, the Flora family, which has a similar composition, corresponding to LL chondrite meteorites. Out of ${\sim}3380$ NEOs larger or…

Earth and Planetary Astrophysics · Physics 2026-04-08 M. Brož , R. P. Binzel , P. Vernazza , M. Marsset , O. Chrenko , J. Ďurech , D. Herald

The aim is to show that in case of low probability of asteroid collision with Earth, the appropriate selection and weighing of the data are crucial for the impact investigation, and to analyze the impact possibilities using extensive…

Earth and Planetary Astrophysics · Physics 2015-05-13 Malgorzata Krolikowska , Grzegorz Sitarski , Andrzej M. Soltan

We present orbital integrations for various Jupiter family comets (JFCs) in the 55 Cancri system. This star is known to possess (at least) five planets with masses ranging from super-Earth to Jupiter-type. Furthermore, according to…

Earth and Planetary Astrophysics · Physics 2020-06-24 Rudolf Dvorak , Birgit Loibnegger , Manfred Cuntz

DESTINY+ is an upcoming JAXA Epsilon medium-class mission to fly by the Geminids meteor shower parent body (3200) Phaethon. It will be the world's first spacecraft to escape from a near-geostationary transfer orbit into deep space using a…

Based on currently available kinematic data, we have searched for stars outside the Hipparcos list that either closely encountered in the past or will encounter in the future the Solar system within several parsecs. For the first time, we…

Solar and Stellar Astrophysics · Physics 2015-05-20 Vadim V. Bobylev

Following the suggestion of Black (1997) that some massive extrasolar planets may be associated with the tail of the distribution of stellar companions, we investigate a scenario in which 5 < N < 100 planetary mass objects are assumed to…

Astrophysics · Physics 2009-10-31 J. C. B. Papaloizou , Caroline Terquem