Issue |
EPJ Web of Conferences
Volume 16, 2011
Research, Science and Technology of Brown Dwarfs and Exoplanets: Proceedings of an International Conference held in Shangai on Occasion of a Total Eclipse of the Sun
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Article Number | 06006 | |
Number of page(s) | 3 | |
Section | Very Low-Mass Stars and Brown Dwarfs | |
DOI | https://doi.org/10.1051/epjconf/20111606006 | |
Published online | 18 July 2011 |
https://doi.org/10.1051/epjconf/20111606006
TNO, occultation, and high angular resolution astronomy
Institute of Astronomy and Astrophysics, Academia Sinica, PO Box 23-141, Taipei 106, Taiwan, R.O.C.
a e-mail: skking@asiaa.sinica.edu.tw
The trans-Neptunian region is a new frontier in the solar system research. Occultation is currently the only way to detect a trans-Neptunian object (TNO) of typical comet-size in that region. By monitoring thousands of stars at a cadence of about 10 Hz, any TNO event will enable astrometry at sub-milli-arcsec level. The status of related researches is summarized.
© Owned by the authors, published by EDP Sciences, 2011
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