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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

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

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

The near-Earth asteroid 3200 Phaethon (1983 TB) is an attractive object not only from a scientific viewpoint but also because of JAXA's DESTINY+ target. The rotational lightcurve and spin properties were investigated based on the data…

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…

(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

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

(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

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,…

We present a deep imaging and spectroscopic search for emission from (3200) Phaethon, a large near-Earth asteroid that appears to be the parent of the strong Geminid meteoroid stream, using the 4.3 m Lowell Discovery Telescope. Observations…

地球与行星天体物理 · 物理学 2020-11-23 Quanzhi Ye , Matthew M. Knight , Michael S. P. Kelley , Nicholas A. Moskovitz , Annika Gustafsson , David Schleicher

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 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…

We present an analysis of asteroid (3200) Phaethon using coronagraphic observations from 2008 to 2022 by the COR2 cameras onboard the twin Solar TErrestrial RElations Observatory (STEREO) spacecraft. Although undetected in individual…

地球与行星天体物理 · 物理学 2023-02-15 Man-To Hui

We present JWST observations of the near-Earth asteroid (3200) Phaethon using the Near-Infrared Camera (NIRCam), Near-Infrared Spectrograph (NIRSpec), and Mid-Infrared Instrument (MIRI) to further investigate the composition of Phaethon's…

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 present a study of planet-crossing asteroid (3200) Phaethon at three successive perihelia in 2009, 2010 and 2012, using the NASA STEREO spacecraft. Phaethon is clearly detected in 2009 and 2012, but not in 2010. In both former years,…

地球与行星天体物理 · 物理学 2015-06-15 Jing Li , David Jewitt

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 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…

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