A new asteroid-associated meteor shower and notes on comet-asteroid connection |
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Authors: | H Meng J Zhu X Gong B Yang M Guan D Xia |
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Institution: | a Room 610, Building 45B, School of Physics, Peking University, 5 Yiheyuan Road, Haidian District, Beijing 100871, China b Beijing Planetarium, 38 Xizhimenwai Street, Beijing 100044, China c National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Beijing 100012, China d Department of Physics, Beijing Normal University, Beijing 100875, China e Institute of Geology, China Seismology Bureau, Beijing 100029, China f Department of Astronomy, Beijing Normal University, Beijing 100875, China g National Satellite Meteorological Center, China Meteorological Administration, 46 Zhongguancunnan Street, Beijing 100081, China h Department of Material Science and Engineering, Tsinghua University, Beijing 100084, China i Present address: Department of Metals and Material Engineering, University of British Columbia, 309-6350 Stores Road, Vancouver, BC, Canada V6T 1Z4 j Space Exploration Magazine, Building 1, 2 Yuetanbeixiaojie, Beijing 100830, China |
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Abstract: | The calculation of the orbit of the potentially hazardous Asteroid 2001 YB5 suggests a possible meteor shower around January 7.5, 2002 UT. Video observations revealed an unidentified radiant around the predicted maximum time, at RA=121.5°, Dec=+11.5°(for solar longitude 287.30°). Visual observers also reported unusually high rates from that region on the same night, indicating that 2001 YB5 did produce a weak meteor shower. Furthermore, it is noticed that 2001 YB5 is a rare B-type asteroid in same spectral class with Asteroid (3200) Phaethon, the parent body of the only previously known asteroid-associate meteor shower, Geminids. |
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Keywords: | Asteroids Comets Meteors |
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