中文
相关论文

相关论文: The Wagging Plasma Tail of Comet C/2020 S3 (Erasmu…

200 篇论文

Context. The occultation of a radio source by the plasma tail of a comet can be used to probe structure and dynamics in the tail. Such occultations are rare, and the occurrence of scintillation, due to small-scale density variations in the…

地球与行星天体物理 · 物理学 2022-11-09 R. A. Fallows , B. Forte , M. Mevius , M. A. Brentjens , C. G. Bassa , M. M. Bisi , A. Offringa , G. Shaifullah , C. Tiburzi , H. Vedantham , P. Zucca

We identified a new ultra-distant comet C/2019 E3 (ATLAS) exhibiting preperihelion cometary activity at heliocentric distances $\gtrsim\!20$ au, making it the fourth member of this population after C/2010 U3 (Boattini), C/2014 UN$_{271}$…

地球与行星天体物理 · 物理学 2024-01-10 Man-To Hui , Robert Weryk , Marco Micheli , Zhong Huang , Richard Wainscoat

We describe the physical and orbital properties of C/2011 W3. After surviving perihelion, the comet underwent major changes (permanent loss of nuclear condensation, formation of spine tail). The process of disintegration culminated with an…

地球与行星天体物理 · 物理学 2015-06-05 Zdenek Sekanina , Paul W. Chodas

We report the electron density in a plasma tail of Comet ISON (C/2012 S1) derived from interplanetary scintillation (IPS) observations during November 1--28, 2013. Comet ISON showed a well-developed plasma tail (longer than 2.98 x 10^{7}…

地球与行星天体物理 · 物理学 2015-03-02 Tomoya Iju , Shinsuke Abe , Munetoshi Tokumaru , Ken'ichi Fujiki

We combine ground- and space-based observations of long-period comet C/2021 O3 (Panstarrs) (perihelion distance 0.287 au) in order to investigate its reported near-perihelion destruction. Pre-perihelion photometric observations show a…

地球与行星天体物理 · 物理学 2025-06-12 David Jewitt. Jing Li , Michael Jaeger , Yoonyoung Kim

A morphological and photometric analysis of the naked-eye long-period comet C/2022 E3 (ZTF) before perihelion is presented in this study. The observation images taken by the Zwicky Transient Facility survey telescope from July 2022 to…

地球与行星天体物理 · 物理学 2024-05-27 Bin Liu , Xiaodong Liu

Long-period comets are planetesimal remnants constraining the environment and volatiles of the protoplanetary disc. We report the discovery of hyperbolic long-period comet C/2022 E3 (ZTF), which has a perihelion $\sim$1.11 au, an…

The close encounter of Comet C/2013 A1 (Siding Spring) with Mars on October 19, 2014 presented an extremely rare opportunity to obtain the first flyby quality data of the nucleus and inner coma of a dynamically new comet. However, the…

We present observations of the detection of a faint high-latitude jet in the inner coma of comet 3I/ATLAS that coincides with the broad plume detected in visible images along PA $280 \pm 10^{\circ}$. A detailed analysis shows that the jet…

地球与行星天体物理 · 物理学 2025-12-16 M. Serra-Ricart , J. Licandro , M. R. Alarcon

Context. During their journey to perihelion, comets may appear in the field-of-view of space-borne optical instruments, showing in some cases a nicely developed plasma tail extending from their coma and exhibiting an oscillatory behaviour.…

地球与行星天体物理 · 物理学 2018-08-08 G. Nisticò , V. Vladimirov , V. M. Nakariakov , K. Battams , V. Bothmer

In 2021 and 2022 the hydrogen comae of three long period comets, C/2020 S3 (Erasmus), C/2021 A1 (Leonard) and C/2021 O3 (PanSTARRS) were observed with the Solar Wind ANisotropies (SWAN) all-sky hydrogen Lyman-alpha camera on the SOlar and…

地球与行星天体物理 · 物理学 2023-04-10 M. R. Combi , T. Mäkinen , J. -L. Bertaux , E. Quémerais , S. Ferron

Comet C/2025 K1 (ATLAS) reached perihelion at 0.33 au on 2025 October 8. Daily monitoring by the LCO Outbursting Objects Key Project revealed a major activity increase between November 2 and 4, accompanied by rapid changes in coma…

We report short-time variations in the plasma tail of C/2013 R1(Lovejoy). A series of short (two to three minutes) exposure images with the 8.2-m Subaru telescope shows faint details of filaments and their motions over 24 minutes observing…

地球与行星天体物理 · 物理学 2015-06-19 Masafumi Yagi , Jin Koda , Reiko Furusho , Tsuyoshi Terai , Hideaki Fujiwara , Jun-ichi Watanabe

The 2023 perihelion passage of comet C/2022 E3 (ZTF) afforded an opportunity to measure the abundances and spatial distributions of coma volatiles in an Oort cloud comet at high spatial resolution near its close approach to Earth…

The recent close approach of comet C/2020 F3 (NEOWISE) allowed us to study the morphology of its inner coma. From the measurement of the dust ejection velocityon spiral structures expanding around the nucleus, we estimated a mean…

地球与行星天体物理 · 物理学 2021-09-07 F. Manzini , V. Oldani , P. Ochner , E. Barbotin , L. R. Bedin , R. Behrend , G. Fardelli

We present our results for comet (ISON). Our results were obtained with amateur telescopes observing from the ground, before and after the comet had passed conjunction with the Sun in August 2013. We measured a mean radius of 830 +- 245 m,…

太阳与恒星天体物理 · 物理学 2014-05-14 Toni Scarmato

Comet C/2002 S2, a member of the Kreutz family of Sungrazing comets, was discovered in white light images of the SOHO/LASCO coronagraph on 2002 September 18 and observed in \hi\, \lya\, emission by the SOHO/UVCS instrument at four different…

太阳与恒星天体物理 · 物理学 2015-06-23 Silvio Giordano , John C. Raymond , Philippe Lamy , Michael Uzzo , Danuta Dobrzycka

Imaging polarimetry enables the spatially resolved investigation of cometary dust properties across different morphological structures. While cometary comae have been studied thoroughly in the pertinent literature, cometary tails have…

地球与行星天体物理 · 物理学 2026-03-11 Mirza Arnaut , Christian Wöhler , Pritish Halder , Goldy Ahuja , Shashikiran Ganesh , Megha Bhatt

We report results from broadband visible images of comet C/2012 S1 (ISON) obtained with the Hubble Space Telescope Wide Field Camera 3 on 2013 April 10. C/ISON's coma brightness follows a 1/{\rho} (where {\rho} is the projected distance…

We present a photometric and dynamical study of comet C/2010 U3 (Boattini), which was seen active in prediscovery data as early as 2005 November at a new inbound record heliocentric distance $r_{\rm H} = 25.8$ au. Two outburst events around…

地球与行星天体物理 · 物理学 2019-04-17 Man-To Hui , Davide Farnocchia , Marco Micheli
‹ 上一页 1 2 3 10 下一页 ›