𝔖 Bobbio Scriptorium
✦   LIBER   ✦

EURONEAR: Data mining of asteroids and Near Earth Asteroids

✍ Scribed by O. Vaduvescu; L. Curelaru; M. Birlan; G. Bocsa; L. Serbanescu; A. Tudorica; J. Berthier


Publisher
John Wiley and Sons
Year
2009
Tongue
English
Weight
284 KB
Volume
330
Category
Article
ISSN
0004-6337

No coin nor oath required. For personal study only.

✦ Synopsis


Abstract

Besides new observations, mining old photographic plates and CCD image archives represents an opportunity to recover and secure newly discovered asteroids, also to improve the orbits of Near Earth Asteroids (NEAs), Potentially Hazardous Asteroids (PHAs) and Virtual Impactors (VIs). These are the main research aims of the EURONEAR network. As stated by the IAU, the vast collection of image archives stored worldwide is still insufficiently explored, and could be mined for known NEAs and other asteroids appearing occasionally in their fields. This data mining could be eased using a server to search and classify findings based on the asteroid class and the discovery date as β€œprecoveries” or β€œrecoveries”. We built PRECOVERY, a public facility which uses the Virtual Observatory SkyBoT webservice of IMCCE to search for all known Solar System objects in a given observation. To datamine an entire archive, PRECOVERY requires the observing log in a standard format and outputs a database listing the sorted encounters of NEAs, PHAs, numbered and un‐numbered asteroids classified as precoveries or recoveries based on the daily updated IAU MPC database. As a first application, we considered an archive including about 13 000 photographic plates exposed between 1930 and 2005 at the Astronomical Observatory in Bucharest, Romania. Firstly, we updated the database, homogenizing dates and pointings to a common format using the JD dating system and J2000 epoch. All the asteroids observed in planned mode were recovered, proving the accuracy of PRECOVERY. Despite the large field of the plates imaging mostly 2.27Β° Γ— 2.27Β° fields, no NEA or PHA could be encountered occasionally in the archive due to the small aperture of the 0.38m refractor insufficiently to detect objects fainter than V ∼ 15. PRECOVERY can be applied to other archives, being intended as a public facility offered to the community by the EURONEAR project. This is the first of a series of papers aimed to improve orbits of PHAs and NEAs using precovered data derived from archives of images to be data mined in collaboration with students and amateurs. In the next paper we will search the CFHT Legacy Survey, while data mining of other archives is planned for the near future (Β© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)


πŸ“œ SIMILAR VOLUMES


Lightcurves of 7 Near-Earth Asteroids
✍ Petr Pravec; Lenka Ε arounovΓ‘; Marek Wolf πŸ“‚ Article πŸ“… 1996 πŸ› Elsevier Science 🌐 English βš– 292 KB
Lightcurves of 26 Near-Earth Asteroids
✍ Petr Pravec; Marek Wolf; Lenka Ε arounovΓ‘ πŸ“‚ Article πŸ“… 1998 πŸ› Elsevier Science 🌐 English βš– 969 KB
The D Discriminant and Near-Earth Astero
✍ Jack D. Drummond πŸ“‚ Article πŸ“… 2000 πŸ› Elsevier Science 🌐 English βš– 698 KB

A method of separating an association of orbits, a stream, from the local background using the traditional D discriminant is introduced. Applying this procedure to all 708 asteroids with perihelia less than 1.3 AU known on April 22, 1999 suggests that the orbits of Earth-approaching asteroids may be

The Size and Shape of the Near-Earth Ast
✍ David L. Rabinowitz πŸ“‚ Article πŸ“… 1994 πŸ› Elsevier Science 🌐 English βš– 807 KB

Evidence was recently reported for the existence of a near-Earth belt of small, Earth-approaching asteroids (SEAs) with diameters less than \(\sim \mathbf{5 0} \mathrm{m}\). This result was based upon observations made with the Spacewatch Telescope of the University of Arizona during the course of a

Physical Characteristics of Near-Earth A
✍ Alan W. Harris; John K. Davies πŸ“‚ Article πŸ“… 1999 πŸ› Elsevier Science 🌐 English βš– 156 KB

Thermal infrared spectrophotometric observations of the near-Earth asteroids 433 Eros, 1980 Tezcatlipoca, and 3671 Dionysus are presented and their implications for the physical characteristics of the objects discussed. Sizes and albedos are derived on the basis of published thermal models and compa