activity
20132025
most citedOptical observations of NEA 3200 Phaethon (1983 TB) during the 2017 apparition

20 citations · 120 across the 15 of their papers we have counts for

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15 papers · 1 filter

astro-ph.EP2025★ 6 cited

Discovery and dynamics of a Sedna-like object with a perihelion of 66 au

Ying-Tung Chen, Patryk Sofia Lykawka, Yukun Huang +30

Trans-Neptunian objects (TNOs) with large perihelion distances ( au) and semi-major axes ( au) provide insights into the early evolution of the solar system and th…

astro-ph.EP2023★ 1 cited

Photometry of the Didymos system across the DART impact apparition

Nicholas Moskovitz, Cristina Thomas, Petr Pravec +78

On 26 September 2022, the Double Asteroid Redirection Test (DART) spacecraft impacted Dimorphos, the satellite of binary near-Earth asteroid (65803) Didymos. This demonstrated the…

astro-ph.EP2021★ 5 cited

A new approach to feature-based asteroid taxonomy in 3D color space: 1. SDSS photometric system

Dong-Goo Roh, Hong-Kyu Moon, Min-Su Shin +1

The taxonomic classification of asteroids has been mostly based on spectroscopic observations with wavelengths spanning from the VIS to the NIR. VIS-NIR spectra of 2500 aster…

astro-ph.EP2021★ 18 cited

Rotation acceleration of asteroids (10115) 1992 SK, (1685) Toro, and (1620) Geographos due to the YORP effect

J. Durech, D. Vokrouhlicky, P. Pravec +28

The rotation state of small asteroids is affected by the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect, which is a net torque caused by solar radiation directly reflected and…

astro-ph.EP2021

FOSSIL: I. The Spin Rate Limit of Jupiter Trojans

Chan-Kao Chang, Ying-Tung Chen, Wesley C. Fraser +25

Rotation periods of 53 small (diameters km) Jupiter Trojans (JTs) were derived using the high-cadence light curves obtained by the FOSSIL phase I survey, a Subaru/Hype…

astro-ph.EP2020★ 11 cited

Spin Change of Asteroid 2012 TC4 probably by Radiation Torques

Hee-Jae Lee, Josef Ďurech, David Vokrouhlický +9

Asteroid 2012 TC4 is a small (10 m) near-Earth object that was observed during its Earth close approaches in 2012 and 2017. Earlier analyses of light curves revealed its exci…

astro-ph.EP2020★ 4 cited

Shape model and spin state of non-principal axis rotator (5247) Krylov

H. -J. Lee, J. Ďurech, M. -J. Kim +12

Context. The study of non-principal axis (NPA) rotators can provide important clues to the evolution of the spin state of asteroids. However, so far, very few studies have focused…

astro-ph.EP2019

The Geometric Albedo of (4179) Toutatis Estimated from KMTNet DEEP-South Observations

Yoonsoo P. Bach, Masateru Ishiguro, Sunho Jin +6

We derive the geometric albedo of a near-Earth asteroid, (4179) Toutatis, to investigate its surface physical conditions. The asteroid has been studied rigorously not only via grou…

astro-ph.EP2019★ 4 cited

ASIME 2018 White Paper. In-Space Utilisation of Asteroids: Asteroid Composition -- Answers to Questions from the Asteroid Miners

Amara L. Graps, Angel Abbud-Madrid, Paul Abell +41

In keeping with the Luxembourg government's initiative to support the future use of space resources, ASIME 2018 was held in Belval, Luxembourg on April 16-17, 2018. The goal of ASI…

astro-ph.EP2018★ 12 cited

Investigation of surface homogeneity of (3200) Phaethon

Hee-Jae Lee, Myung-Jin Kim, Dong-Heun Kim +7

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 Phaetho…

astro-ph.EP2018★ 20 cited

Optical observations of NEA 3200 Phaethon (1983 TB) during the 2017 apparition

Myung-Jin Kim, Hee-Jae Lee, Sang-Min Lee +24

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 a…

astro-ph.EP2017★ 5 cited

Shape and spin determination of Barbarian asteroids

M. Devogèle, P. Tanga, P. Bendjoya +51

Context. The so-called Barbarian asteroids share peculiar, but common polarimetric properties, probably related to both their shape and composition. They are named after (234) Barb…

astro-ph.EP2017★ 13 cited

Confirmation of Large Super-Fast Rotator (144977) 2005 EC127

Chan-Kao Chang, Hsing-Wen Lin, Wing-Huen Ip +7

(144977) 2005 EC127 is an V-/A-type inner-main-belt asteroid with a diameter of 0.6 +- 0.1 km. Asteroids of this size are believed to have rubble-pile structure, and, therefore, ca…

astro-ph.EP2013★ 8 cited

Rotational properties of Maria asteroid family

Myung-Jin Kim, Young-Jun Choi, Hong-Kyu Moon +13

Maria family is regarded as an old-type (~3 +/- 1 Gyr) asteroid family which has experienced substantial collisional and dynamical evolution in the Main-belt. It is located nearby…

astro-ph.EP2013★ 13 cited

Optical observations of NEA 162173 (1999 JU3) during the 2011-2012 apparition

M. -J. Kim, Y. -J. Choi, H. -K. Moon +7

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 aster…