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A variety of supernova events, including Type IIn supernovae and ultraluminous supernovae, appear to have lost up to solar masses of their envelopes in 10's to 100's of years leading up to the explosion. In order to explain the close timing…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Roger A. Chevalier

The Sun is located in a low-density region of the interstellar medium partially filled with hot gas that is the likely result of several nearby supernova explosions within the last 10 Myr. Here we use astrometric data to show that part of…

Astrophysics · Physics 2016-08-16 Jesús Maíz-Apellániz

Gas-giant planets, like Jupiter and Saturn, acquire massive gaseous envelopes during the approximately 3 Myr-long lifetimes of protoplanetary discs. In the core accretion scenario, the formation of a solid core of around 10 Earth masses…

Earth and Planetary Astrophysics · Physics 2019-09-25 Michiel Lambrechts , Elena Lega , Richard P. Nelson , Aurélien Crida , Alessandro Morbidelli

We provide evidence that the obliquities of stars with close-in giant planets were initially nearly random, and that the low obliquities that are often observed are a consequence of star-planet tidal interactions. The evidence is based on…

It is well accepted that 'hot Jupiters' did not form in situ, as the temperature in the protoplanetary disc at the radius at which they now orbit would have been too high for planet formation to have occurred. These planets, instead, form…

Earth and Planetary Astrophysics · Physics 2015-06-05 W. K. M. Rice , J. Veljanoski , A. Collier Cameron

Evidence for cometary activity beyond Jupiter and Saturn's orbits -- such as that observed for Centaurs and long period comets -- suggests that the thermal processing of comet nuclei starts long before they enter the inner Solar System,…

Earth and Planetary Astrophysics · Physics 2022-04-06 Anastasios Gkotsinas , Aurélie Guilbert-Lepoutre , Sean N. Raymond , David Nesvorný

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

Detecting heat from minor planets in the outer solar system is challenging, yet it is the most efficient means for constraining the albedos and sizes of Kuiper Belt Objects (KBOs) and their progeny, the Centaur objects. These physical…

The last three decades the asteroid (1) Ceres is an object of the intensive ground-and space-based observations. A new unusual contributing to these studies represents the recent detection of localized sources of water vapour releasing from…

General Physics · Physics 2014-04-10 Yury I. Rogozin

A posteriori anisotropy study of ultra-high energy cosmic rays (UHECRs) with the Pierre Auger Observatory (PAO) has shown evidence of excess of cosmic ray particles above 55 EeV within $18^{\circ}$ of the direction of the radio galaxy…

High Energy Astrophysical Phenomena · Physics 2015-06-05 Ruo-Yu Liu , Xiang-Yu Wang , Wei Wang , A. M. Taylor

Cometary activity is a manifestation of sublimation-driven processes at the surface of nuclei. However, cometary outbursts may arise from other processes that are not necessarily driven by volatiles. In order to fully understand nuclear…

Proxima Centauri b, an Earth-size planet in the habitable zone of our nearest stellar neighbour, has just been discovered. A theoretical framework of synchronously rotating planets, in which the risk of a runaway greenhouse on the sunlight…

Earth and Planetary Astrophysics · Physics 2016-08-26 Colin Goldblatt

The asteroid belt was dynamically shaped during and after planet formation. Despite representing a broad ring of stable orbits, the belt contains less than one one-thousandth of an Earth mass. The asteroid orbits are dynamically excited…

Earth and Planetary Astrophysics · Physics 2022-07-20 Sean N. Raymond , David Nesvorny

Our knowledge of main-belt comets (MBCs), which exhibit comet-like activity likely due to the sublimation of volatile ices, yet orbit in the main asteroid belt, has increased greatly since the discovery of the first known MBC,…

Earth and Planetary Astrophysics · Physics 2016-03-16 Henry H. Hsieh

We report the detection of water ice in the Centaur 2060 Chiron, based on near-infrared spectra (1.0 - 2.5 micron) taken with the 3.8-meter United Kingdom Infrared Telescope (UKIRT) and the 10-meter Keck Telescope. The appearance of this…

Astrophysics · Physics 2009-10-31 J. X. Luu , D. C. Jewitt , C. Trujillo

We performed a monitoring observation of a Jupiter-Family comet, 17P/Holmes, during its 2014 perihelion passage to investigate its secular change in activity. The comet has drawn the attention of astronomers since its historic outburst in…

Activity of most comets near the Sun is dominated by sublimation of frozen water, the most abundant ice in comets. Some comets, however, are active well beyond the water-ice sublimation limit of ~3 AU. Three bodies dominate the…

Earth and Planetary Astrophysics · Physics 2017-03-23 Maria Womack , Gal Sarid , Kacper Wierzchos

Main Belt comets represent a recently discovered class of objects. They are quite intriguing because, while having a Tisserand invariant value higher than 3, are showing cometary activity. We study the activity of the Main Belt comets…

Earth and Planetary Astrophysics · Physics 2015-06-03 Maria Teresa Capria , Simone Marchi , Maria Cristina De Sanctis , Angioletta Coradini , Eleonora Ammannito

So-called 'dark comets' are small, morphologically inactive near-Earth objects (NEOs) that exhibit nongravitational accelerations inconsistent with radiative effects. These objects exhibit short rotational periods (minutes to hours), where…

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