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相关论文: Optical observations of NEA 3200 Phaethon (1983 TB…

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(3200) Phaethon exhibits both comet- and asteroid-like properties, suggesting it could be a rare transitional object such as a dormant comet or previously volatile-rich asteroid. This justifies detailed study of (3200) Phaethon's physical…

地球与行星天体物理 · 物理学 2015-06-22 Megan Ansdell , Karen J. Meech , Olivier Hainaut , Marc W. Buie , Heather Kaluna , James Bauer , Luke Dundon

The near-Earth asteroid (3200) Phaethon is an intriguing object: its perihelion is at only 0.14 au and is associated with the Geminid meteor stream. We aim to use all available disk-integrated optical data to derive a reliable convex shape…

Asteroid (3200) Phaethon is a Near-Earth Apollo asteroid with an unusual orbit that brings it closer to the Sun than any other known asteroid. Its last close approach to the Earth was in mid-December 2017 and the next one will be on October…

We present results of polarimetric, photometric, and spectral observations of the near-Earth asteroid (3200) Phaethon carried out at the 6-m BTA telescope of the Special Astrophysical Observatory and the 2.6-m and 1.25-m telescopes of the…

地球与行星天体物理 · 物理学 2022-07-06 N. Kiselev , V. Rosenbush , D. Petrov , I. Luk'yanyk , O. V. Ivanova , N. V. Pit , K. A. Antoniuk , V. L. Afanasiev

The recent close approach of the NEA (3200) Phaethon offered a rare opportunity to obtain high-quality observational data. We used the newly obtained optical light curves to improve the spin and shape model of Phaethon and to determine its…

The main aim of photometrical observations of the asteroid 3200 Phaethon was searching for its low-level cometary activity (possible coma and/or dust tail) in the pre-perihelion passage. We performed observational runs with telescopes…

地球与行星天体物理 · 物理学 2019-06-05 A. Kartashova , M. Husarik , O. Ivanova , G. Kokhirova , E. Bakanas , I. Sokolov , U. Kh. Khamroev , A. A. Ibragimov

Accurate estimation of brightness of (3200) Phaethon up to lower phase angles are essential for planning of the on-board camera of the DESTINY$^{+}$ mission. We have carried out intensive observations of Phaethon in the optical wavelength…

We report on a multi-observatory campaign to examine asteroid 3200 Phaethon during its December 2017 close approach to Earth, in order to improve our measurements of its fundamental parameters, and to search for surface variations, cometary…

地球与行星天体物理 · 物理学 2019-07-10 Maryam Tabeshian , Paul Wiegert , Quanzhi Ye , Man-To Hui , Xing Gao , Hanjie Tan

(3200) Phaethon is a compelling object as it has an asteroidal appearance and spectrum, produces a weak dust tail during perihelion at just 0.14 AU, and is the parent body of the Geminid Meteor Shower. A better understanding of the physical…

地球与行星天体物理 · 物理学 2018-12-05 Theodore Kareta , Vishnu Reddy , Carl Hergenrother , Dante S. Lauretta , Tomoko Arai , Driss Takir , Juan Sanchez , Josef Hanuš

Context. (3200) Phaethon is a ~5-km-diameter near-Earth asteroid with a small perihelion distance of 0.14 au and is the parent body of the Geminids. JAXA's DESTINY+ mission will fly by Phaethon in the near future. Aims. We aim to support…

地球与行星天体物理 · 物理学 2025-04-02 Hangbin Jo , Masateru Ishiguro , Derek C. Richardson , Sean E. Marshall , Tomoko Arai , Ko Ishibashi

We report on the first polarimetric study of (3200) Phaethon, the target of JAXA's DESTINY$^+$ mission, in the negative branch to ensure its anhydrous nature and to derive an accurate geometric albedo. We conducted observations at low phase…

Apollo-type NEA (3200) Phaethon, classified at the B/F-type taxonomy, probably the main mass of the Phaethon-Geminid stream complex (PGC), can be the most metamorphic C-complex asteroid in our solar system, since it is heated up to ~1000 K…

地球与行星天体物理 · 物理学 2017-03-02 Daisuke Kinoshita , Katsuhito Ohtsuka , Takashi Ito , Seidai Miyasaka , Tomoki Nakamura , Shinsuke Abe , Wen-Ping Chen

Near-Earth asteroid (3200) Phaethon is notable for its association to a strong annual meteor shower, the Geminids, indicative of one or more episodes of mass ejection in the past. The mechanism of Phaethon's past activity is not yet…

地球与行星天体物理 · 物理学 2018-09-05 Quanzhi Ye , Paul A. Wiegert , Man-To Hui

Time-series multi-band photometry and spectrometry were performed in Nov.-Dec. 2017 to investigate the homogeneity of the surface of asteroid (3200) Phaethon. We found that Phaethon is a B-type asteroid, in agreement with previous studies,…

(155140) 2005 UD has a similar orbit to (3200) Phaethon, an active asteroid in a highly eccentric orbit thought to be the source of the Geminid meteor shower. Evidence points to a genetic relationship between these two objects, but we have…

We present a study of the active asteroid (3200) Phaethon in the 2016 apparition using the STEREO spacecraft and compare the results with data from the previous two perihelia in 2009 and 2012. Once again, Phaethon brightened by $\sim$2 mag…

地球与行星天体物理 · 物理学 2016-12-28 Man-To Hui , Jing Li

We present Hubble Space Telescope observations of the active asteroid (and Geminid stream parent) 3200 Phaethon when at its closest approach to Earth (separation 0.07 AU) in 2017 December. Images were recorded within $\sim$1\degr~of the…

地球与行星天体物理 · 物理学 2018-11-07 David Jewitt , Max Mutchler , Jessica Agarwal , Jing Li

We report Arecibo S-band (2380 MHz; 12.6 cm) radar observations of near-Earth asteroid (3200) Phaethon during the December 2017 apparition when Phaethon passed within 0.07 au of Earth. Radar images with a resolution of 75 m per pixel reveal…

We report on optical polarimetric observations of two Apollo type near-Earth asteroids, (422699) 2000 PD3 and (3200) Phaethon, and BVRI photometric observations of 2000 PD3 using the 1.6m Pirka telescope in 2017. We derived the geometric…

Near-Earth asteroid 162173 (1999 JU3) is a potential target of two asteroid sample return missions, not only because of its accessibility but also because of the first C-type asteroid for exploration missions. The lightcurve-related…

地球与行星天体物理 · 物理学 2015-06-15 M. -J. Kim , Y. -J. Choi , H. -K. Moon , M. Ishiguro , S. Mottola , M. Kaplan , D. Kuroda , D. S. Warjurkar , J. Takahashi , Y. -I. Byun
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