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1I/`Oumuamua is the first known interstellar small body, probably being only about 100~m in size. Against expectations based on comets, `Oumuamua does not show any activity and has a very elongated figure, and also exhibits undamped…

地球与行星天体物理 · 物理学 2018-01-10 Matija Ćuk

At present, there exists no consensus in the astronomical community regarding either the bulk composition or the formation mechanism for the interstellar object 1I/2017 U1 ('Oumuamua). With the goal of assessing the merits of the various…

地球与行星天体物理 · 物理学 2021-11-24 W. Garrett Levine , Samuel H. C. Cabot , Darryl Seligman , Gregory Laughlin

The first known interstellar object 'Oumuamua exhibited a nongravitational acceleration that appeared inconsistent with cometary outgassing, leaving radiation pressure as the most likely force. Bar the alien lightsail hypothesis, an…

地球与行星天体物理 · 物理学 2020-01-08 Eirik G. Flekkøy , Jane X. Luu , Renaud Toussaint

The properties of the first-discovered interstellar object (ISO), 1I/2017 (`Oumuamua), differ from both Solar System asteroids and comets, casting doubt on a protoplanetary disk origin. In this study, we investigate the possibility that it…

地球与行星天体物理 · 物理学 2021-05-05 W. Garrett Levine , Gregory Laughlin

`Oumuamua (1I/2017 U1) is the first object of interstellar origin observed in the Solar System. Recently, \citet{Micheli2018} reported that `Oumuamua showed deviations from a Keplerian orbit at a high statistical significance. The observed…

地球与行星天体物理 · 物理学 2018-11-28 Shmuel Bialy , Abraham Loeb

I present a re-analysis of the available observational constraints on the trajectory of 'Oumuamua, the first confirmed interstellar object discovered in the solar system. 'Oumuamua passed through the inner solar system on a hyperbolic…

地球与行星天体物理 · 物理学 2023-04-17 Federico Spada

The origin of the interstellar object 1I/'Oumuamua, has defied explanation. In a companion paper (Jackson & Desch, 2021), we show that a body of N2 ice with axes 45 m x 44 m x 7.5 m at the time of observation would be consistent with its…

地球与行星天体物理 · 物理学 2021-06-02 Steven J. Desch , Alan P. Jackson

Interstellar comets penetrating through the Solar System had been anticipated for decades. The discovery of asteroidal-looking 'Oumuamua was thus a huge surprise and a puzzle. Furthermore, the physical properties of the 'first scout' turned…

地球与行星天体物理 · 物理学 2019-10-15 Piotr Guzik , Michał Drahus , Krzysztof Rusek , Wacław Waniak , Giacomo Cannizzaro , Inés Pastor-Marazuela

The recently discovered first high velocity hyperbolic objects passing through the Solar System, 1I/'Oumuamua and 2I/Borisov, have raised the question about near term missions to Interstellar Objects. In situ spacecraft exploration of these…

In single star systems like our own Solar system, comets dominate the mass budget of bodies that are ejected into interstellar space, since they form further away and are less tightly bound. However 1I/`Oumuamua, the first interstellar…

地球与行星天体物理 · 物理学 2018-03-30 Alan P. Jackson , Daniel Tamayo , Noah Hammond , Mohamad Ali-Dib , Hanno Rein

Observations of the first interstellar minor object 1I/2017 'Oumuamua did not reveal direct signs of outgassing that would have been natural if it had volatile-rich composition. However, a recent measurement by Micheli et al (2018) of a…

地球与行星天体物理 · 物理学 2018-11-07 Roman R. Rafikov

The detection of Interstellar Objects passing through the Solar System offers the promise of constraining the physical and chemical processes involved in planetary formation in other extrasolar systems. While the effect of outgassing by…

We study the destruction and modification of icy interstellar objects by cosmic rays and gas collisions. Using the cosmic-ray flux measured in the local interstellar medium as well as inferred from gamma-ray observations at the different…

星系天体物理 · 物理学 2021-11-01 Vo Hong Minh Phan , Thiem Hoang , Abraham Loeb

The recently discovered first interstellar object 1I/2017 U1 (`Oumuamua) has brightness that varies by a factor of 10, a range greater than that of any Solar System asteroid, a spectrum characteristic of Type D asteroids, and no evidence of…

地球与行星天体物理 · 物理学 2018-05-16 J. I. Katz

Comets are primitive remnants of the early Solar System whose composition offers fundamental clues to their formation and evolution. High-resolution, broad-wavelength spectroscopy is crucial for identifying volatile species and constraining…

地球与行星天体物理 · 物理学 2025-08-06 A. Alvarez-Candal , J. L. Rizos , L. M. Lara , P. Santos-Sanz , P. J. Gutierrez , J. L. Ortiz , N. Morales

The recent discovery by Pan-STARRS1 of 1I/2017 U1 (`Oumuamua), on an unbound and hyperbolic orbit, offers a rare opportunity to explore the planetary formation processes of other stars, and the effect of the interstellar environment on a…

'Oumuamua, the first bona-fide interstellar planetesimal, was discovered passing through our Solar System on a hyperbolic orbit. This object was likely dynamically ejected from an extrasolar planetary system after a series of close…

地球与行星天体物理 · 物理学 2018-03-14 Sean N. Raymond , Philip J. Armitage , Dimitri Veras , Elisa V. Quintana , Thomas Barclay

'Oumuamua was discovered passing through our Solar System on a hyperbolic orbit. It presents an apparent contradiction, with colors similar to those of volatile-rich Solar System bodies but with no visible outgassing or activity during its…

地球与行星天体物理 · 物理学 2018-04-04 Sean N. Raymond , Philip J. Armitage , Dimitri Veras

The recent observation of interstellar objects, 1I/Oumuamua and 2I/Borisov cross the solar system opened new opportunities for planetary science and planetary defense. As the first confirmed objects originating outside of the solar system,…

天体物理仪器与方法 · 物理学 2020-02-05 Ravi teja Nallapu , Yinan Xu , Abraham Marquez , Tristan Schuler , Jekan Thangavelautham

The first interstellar object, `Oumuamua, was discovered in the Solar System by Pan-STARRS in 2017, allowing for a calibration of the impact rate of interstellar meteors of its size $\sim 100\;$m. The discovery of CNEOS 2014-01-08 allowed…

地球与行星天体物理 · 物理学 2022-04-18 Amir Siraj , Abraham Loeb