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Based on a new version of the Hipparcos catalog and currently available radial velocity data, we have searched for stars that either have encountered or will encounter the solar neighborhood within less than 3 pc in the time interval from…

太阳与恒星天体物理 · 物理学 2010-03-11 Vadim V. Bobylev

Stars which pass close to the Sun can perturb the Oort cloud, injecting comets into the inner solar system where they may collide with the Earth. Using van Leeuwen's re-reduction of the Hipparcos data complemented by the original Hipparcos…

太阳与恒星天体物理 · 物理学 2015-02-25 C. A. L. Bailer-Jones

Close encounters of stars to the Sun could affect life on Earth through gravitational perturbations of comets in the Oort cloud or exposure to ionizing radiation. By integrating orbits through the Galactic potential, I identify which of 33…

太阳与恒星天体物理 · 物理学 2022-08-24 C. A. L. Bailer-Jones

We present a comprehensive characterisation of close stellar encounters in the solar vicinity, with a particular focus on placing the predicted fly-by of GJ~710 in context. This star will come extremely close ($0.0621$\,pc or…

太阳与恒星天体物理 · 物理学 2026-05-19 Eloi Fernandez-Puig , Juan Carlos Morales , Ignasi Ribas , Júlia Laguna-Miralles , Pol Guijosa

Passing stars can perturb the Oort Cloud, triggering comet showers and potentially extinction events on Earth. We combine velocity measurements for the recently discovered, nearby, low-mass binary system WISE J072003.20-084651.2 ("Scholz's…

I report on close encounters of stars to the Sun found in the first Gaia data release (GDR1). Combining Gaia astrometry with radial velocities of around 320 000 stars drawn from various catalogues, I integrate orbits in a Galactic potential…

太阳与恒星天体物理 · 物理学 2018-01-10 C. A. L. Bailer-Jones

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

With orbital periods longer than 200 years, most long-period comets (LPCs) remain undiscovered until they are in-bound towards perihelion. The comets that pass close to Earth's orbit are Potentially Hazardous Objects (PHOs). Those with…

地球与行星天体物理 · 物理学 2024-10-10 Samantha Hemmelgarn , Nicholas Moskovitz , Stuart Pilorz , Peter Jenniskens

We examined the influence of the Hyades star cluster on the possibility of the appearance of long-period comets in the Solar system. It is known that the Hyades cluster is extended along the spatial orbit on tens of parsecs. To our…

太阳与恒星天体物理 · 物理学 2019-11-11 M. D. Sizova , E. S. Postnikova , A. P. Demidov , N. V. Chupina , S. V. Vereshchagin

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…

太阳与恒星天体物理 · 物理学 2015-05-20 Vadim V. Bobylev

A search for close encounters of stars with the Solar System was performed using data from the Gaia\,DR3 catalog. We considered 31 stars with the approach parameter $d_{\rm min}<1$~pc. Among them, 15 stars are appearing as candidates for…

星系天体物理 · 物理学 2023-05-23 Vadim Bobylev , Anisa Bajkova

Aims: A previous study claimed that the star HIP 21539 passed close to the Sun, at a distance of 1.9 pc, around 0.14 Myr ago. We show that this is not the case. Methods: We redetermined the trajectory of the star relative to the Sun using a…

太阳与恒星天体物理 · 物理学 2017-05-24 F. Crifo , C. Soubiran , G. Jasniewicz , D. Katz , P. Sartoretti , P. Panuzzo

Meteor showers on the Earth occur at well known times, and are associated with the decay of comets or other minor bodies whose orbital paths pass close to the Earth's trajectory. On the surface, determining the closest proximity of two…

空间物理 · 物理学 2007-05-23 Shane L. Larson

Since 1950 when Oort published his paper on the structure of the cloud of comets it is believed that stars passing near this hypothetical cometary reservoir play an important role in the dynamical evolution of long period comets and…

地球与行星天体物理 · 物理学 2020-01-08 Rita Wysoczańska , Piotr A. Dybczyński , Małgorzata Królikowska

We have computed trajectories, distances and times of closest approaches to the Sun by stars in the Solar neighbourhood with known position, radial velocity and proper motions. For this purpose we have used a full potential model of the…

地球与行星天体物理 · 物理学 2015-05-30 Juan J. Jimenez-Torres , Barbara Pichardo , George Lake , Henry Throop

We investigate the effect of a dark matter caustic passing through the Solar System. We find, confirming a previous result, that the Sun tracks the caustic surface for some time. We integrate numerically the equations of motion of the Sun…

宇宙学与河外天体物理 · 物理学 2025-01-14 Yuxin Zhao , Antonios Kyriazis , Pierre Sikivie

Interstellar material has been discovered in our Solar System, yet its origins and details of its transport are unknown. Here we present $\alpha$ Centauri as a case study of the delivery of interstellar material to our Solar System.…

地球与行星天体物理 · 物理学 2025-03-10 Cole R. Gregg , Paul A. Wiegert

We have searched for the stars that either encountered in the past or will encounter in the future with the Solar system closer than 2 pc. For this purpose, we took more than 216 000 stars with the measured proper motions and trigonometric…

星系天体物理 · 物理学 2017-06-28 V. V. Bobylev , A. T. Bajkova

Given the inexorable increase in the Sun's luminosity, Earth will exit the habitable zone in ~1 Gyr. There is a negligible chance that Earth's orbit will change during that time through internal Solar System dynamics. However, there is a…

地球与行星天体物理 · 物理学 2023-11-22 Sean N. Raymond , Nathan A. Kaib , Franck Selsis , Herve Bouy

We have shown previously (Bobylev et al 2011) that some of the stars in the Solar neighborhood today may have originated in the same star cluster as the Sun, and could thus be called Solar Siblings. In this work we investigate the…

星系天体物理 · 物理学 2015-01-22 M. Valtonen , A. T. Bajkova , V. V. Bobylev , A. Myllari
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