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相关论文: Modelling the 2022 {\tau}-Herculid outburst

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We have analysed the orbits and ablation characteristics in the atmosphere of 59 earth-impacting fireballs, produced by meteoroids one meter in diameter or larger, described here as meter-scale. Using heights at peak luminosity as a proxy…

地球与行星天体物理 · 物理学 2015-12-23 P. Brown , P. Wiegert , D. Clark , E. Tagliaferri

We present deep imaging observations, orbital dynamics, and dust tail model analyses of the double-component asteroid P/2016 J1 (J1-A and J1-B). The observations were acquired at the Gran Telescopio Canarias (GTC) and the…

The relative abundances of singly-deuterated methanol isotopologues, [CH$_{2}$DOH]/[CH$_{3}$OD], in star-forming regions deviate from the statistically expected ratio of 3. In Orion KL, the nearest high-mass star-forming region to Earth,…

星系天体物理 · 物理学 2022-10-12 Olivia H. Wilkins , Geoffrey A. Blake

(60558) 174P/Echeclus is an unusual object that belongs to a class of minor planets called Centaurs, which may be intermediate between Kuiper Belt Objects and Jupiter Family comets. It is sporadically active throughout its orbit at…

地球与行星天体物理 · 物理学 2017-04-28 Kacper Wierzchos , Maria Womack , Gal Sarid

We reply to criticisms by Desch et al. (2021) regarding our Scientific Reports paper, "Breakup of a long-period comet as the origin of the dinosaur extinction." The background impact rates of main-belt asteroids and long-period comets have…

地球与行星天体物理 · 物理学 2021-05-26 Amir Siraj , Abraham Loeb

Here we report evidence of a large solar filament eruption on 2013, September 29. This smooth eruption, which passed without any previous flare, formed after a two-ribbon flare and a coronal mass ejection towards Earth. The coronal mass…

太阳与恒星天体物理 · 物理学 2015-10-29 J. Palacios , C. Cid , A. Guerrero , E. Saiz , Y. Cerrato

In June 2019 the Earth will approach within 5{\deg} mean anomaly of the centre of the Taurid resonant swarm, its closest post-perihelion encounter with Earth since 1975. This will be the best viewing geometry to detect and place limits on…

地球与行星天体物理 · 物理学 2019-06-05 David L. Clark , Paul Wiegert , Peter G. Brown

Everyday thousands of meteoroids enter the Earth's atmosphere. The vast majority burn up harmlessly during the descent, but the larger objects survive, occasionally experiencing intense fragmentation events, and reach the ground. These…

地球与行星天体物理 · 物理学 2021-06-01 Simone Limonta , Mirko Trisolini , Stefan Frey , Camilla Colombo

Multi-wavelength observations of prominence eruptions provide an opportunity to uncover the physical mechanism of the triggering and the evolution process of the eruption. In this paper, we investigated an erupting prominence on October 14,…

太阳与恒星天体物理 · 物理学 2020-10-07 Haiqing Xu , Jiangtao Su , Jie Chen , Guiping Ruan , Arun Kumar Awasthi , Hongqi Zhang , Mei Zhang , Kaifan Ji , Yuzong Zhang , Jiajia Liu

We investigate the aftermath of a giant quiescent solar filament eruption on December 24, 2023. One feature of the eruption is an extensive fan above the filament channel that is about three times as wide as similar structures that appear…

太阳与恒星天体物理 · 物理学 2025-09-15 Xiaoyan Xie , Katharine Reeves , Chengcai Shen , Nishu Karna , Yan Xu , Christopher Moore , Crisel Suarez , Ritesh Patel , Daniel Seaton

Comet P/2010A2 LINEAR is a good candidate for membership with the Main Belt Comet family. It was observed with several telescopes (ESO NTT, La Silla; Gemini North, Mauna Kea; UH 2.2m, Mauna Kea) from 14 Jan. until 19 Feb. 2010 in order to…

地球与行星天体物理 · 物理学 2015-06-03 O. R. Hainaut , J. Kleyna , G. Sarid , B. Hermalyn , A. Zenn , K. J. Meech , P. H. Schultz , H. Hsieh , G. Trancho , J. Pittichová , B. Yang

During its two years mission around comet 67P/Churyumov-Gerasimenko, ESA's Rosetta spacecraft had the unique opportunity to follow closely a comet in the most active part of its orbit. Many studies have presented the typical features…

We present a detailed analysis of an eruptive event that occurred on early 2019 March 8 in active region AR 12734, to which we refer as the International Women's day event. The event under study is intriguing in several aspects: 1)…

太阳与恒星天体物理 · 物理学 2021-09-01 Dumbovic , M. , Veronig , A. M. , Podladchikova , T. , Thalmann , J. K. , Chikunova , G. , Dissauer , K. , Magdalenic , J. , Temmer , M. , Guo , J. , Samara , E

We present the result of a search for charged Higgs decays of the top quark, produced in $p\bar{p}$ collisions at $\surd s =$ 1.8 TeV. When the charged Higgs is heavy and decays to a tau lepton, which subsequently decays hadronically, the…

高能物理 - 实验 · 物理学 2010-05-12 F. Abe

We present a comprehensive reassessment of the region containing the large smooth patch on comet 9P/Tempel 1, leveraging data from the Deep Impact and Stardust-NExT missions, an updated stereophotoclinometry-based shape model, and numerical…

地球与行星天体物理 · 物理学 2026-04-27 J. L. Rizos , T. L. Farnham , J. Kloos , J. M. Sunshine , J. L. Ortiz

The atmosphere of Triton was probed directly by observing a ground-based stellar occultation on 6 October 2022. This rare event yielded 23 positive light curves collected from 13 separate observation stations contributing to our campaign.…

During its most recent return, comet 12P/Pons-Brooks experienced 14 well-documented outbursts, observed between June 13, 2023, and April 2024, at heliocentric distances ranging from $4.26\,$au to $0.85\,$au. After perihelion, two additional…

地球与行星天体物理 · 物理学 2025-02-06 Maria Gritsevich , Marcin Wesołowski , Alberto J. Castro-Tirado

Recent observations show activity in long-period comet C/2017 K2 at heliocentric distances beyond the orbit of Uranus. With this as motivation, we constructed a simple model that takes a detailed account of gas transport modes and simulates…

地球与行星天体物理 · 物理学 2022-01-19 Naceur Bouziani , David Jewitt

In May 2024, the scientific community observed intense solar eruptions that resulted in a great geomagnetic storm and auroral extension, highlighting the need to document and quantify these events. This study mainly focuses on their…

Supersonic turbulence in molecular clouds is a key agent in generating density enhancements that may subsequently go on to form stars. The stronger the turbulence - the higher the Mach number - the more extreme the density fluctuations are…

星系天体物理 · 物理学 2015-05-18 Chris Brunt