KLENOT - PRACTICAL USE OF SOLAR SYSTEM DYNAMICS IN FOLLOW-UP ASTROMETRY OBSERVATIONS OF SMALL SOLAR SYSTEM BODIES

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00070327%3A_____%2F03%3A00014366" target="_blank" >RIV/00070327:_____/03:00014366 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

KLENOT - PRACTICAL USE OF SOLAR SYSTEM DYNAMICS IN FOLLOW-UP ASTROMETRY OBSERVATIONS OF SMALL SOLAR SYSTEM BODIES

Original language description

The KLENOT project is a project of the Klet Observatory, Czech Republic, devoted to astrometric observations of Near Earth objects, distant objects and comets. The improved effort of the large NEO surveys resulting in an increasing number of newly discovered NEOs calls for continuous follow-up astrometry to secure an accurate orbit determination of discovered bodies first in discovery opposition and then during next apparitions. Considering this urgent need of astrometric follow-up, the fact that many of these targets are fainter then magnitude m_V=20.0m and our results and experience in minor planet and comet CCD astrometry done at Klet since 1993, we decided to bring into operation a new 1-m class facility working on a permanent basis - the KLENOT telescope. The regular observing of the telescope started in March 2002 (the MPC code 246). We discuss here methods and techniques we use for follow-up astrometry. Some of the practical results are also mentioned.

Czech name

KLENOT - PRACTICAL USE OF SOLAR SYSTEM DYNAMICS IN FOLLOW-UP ASTROMETRY OBSERVATIONS OF SMALL SOLAR SYSTEM BODIES

Czech description

The KLENOT project is a project of the Klet Observatory, Czech Republic, devoted to astrometric observations of Near Earth objects, distant objects and comets. The improved effort of the large NEO surveys resulting in an increasing number of newly discovered NEOs calls for continuous follow-up astrometry to secure an accurate orbit determination of discovered bodies first in discovery opposition and then during next apparitions. Considering this urgent need of astrometric follow-up, the fact that many of these targets are fainter then magnitude m_V=20.0m and our results and experience in minor planet and comet CCD astrometry done at Klet since 1993, we decided to bring into operation a new 1-m class facility working on a permanent basis - the KLENOT telescope. The regular observing of the telescope started in March 2002 (the MPC code 246). We discuss here methods and techniques we use for follow-up astrometry. Some of the practical results are also mentioned.

Type

D - Article in proceedings

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

<a href="/en/project/GP205%2F02%2FP114" target="_blank" >GP205/02/P114: Orbital elements and ephemerides determination of small bodies of the solar system</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year

2003

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

The Proceedings of the JOURNEES 2003

ISBN

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ISSN

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e-ISSN

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Number of pages

2

Pages from-to

290-291

Publisher name

Institute of Applied Astronomy of the Russian Academy of Sciences and Observatoire de Paris

Place of publication

France

Event location

St. Petersburg, Russia

Event date

Sep 22, 2003

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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