On 2010 July 18.03 working in remote from Madrid, I've confirmed this recently discovered object which was posted on the NEOCP with the observatory designation RO4B8DB, very low in the sky, at only 15 degrees of elevation an moving fast, at nearly 4 arc seconds per minute, this wouldn't seem an easy target if not for the relative brightness about 17 V, some sixty images of 20 seconds each arranged in three stacks of twenty resulted enough to perform astrometry with good signal to noise ratios and low residuals about 0.5 arc seconds.
References : MPEC 2010-O08
La Cañada Observatory, is an initiative by Juan Lacruz, the observatory started astrometric operations in the summer of 2002, it is registered as station J87 in the Minor Planet Center of the International Astronomical Union.
The Observatory also participates in the studies on minor bodies promoted by the Group on Meteorites, Minor Bodies, and Planetary Sciences of the Institute of Space Sciences (CSIC-IEEC).

Este obra está bajo una licencia de Creative Commons Reconocimiento-NoComercial-SinObraDerivada 2.5 España.
The Observatory also participates in the studies on minor bodies promoted by the Group on Meteorites, Minor Bodies, and Planetary Sciences of the Institute of Space Sciences (CSIC-IEEC).
Este obra está bajo una licencia de Creative Commons Reconocimiento-NoComercial-SinObraDerivada 2.5 España.
Showing posts with label Remote observation. Show all posts
Showing posts with label Remote observation. Show all posts
Monday, July 19, 2010
Monday, July 5, 2010
NEO Confirmation 2010 NG
An object posted on MPCs NEOCP was confirmed on a stack of images taken remotely from Madrid on 2010 July 04. Moving at 6 arc seconds per minute at magnitud 19V didn't seem an easy object however the night was clear enough to allow an early detection with small residuals. Because the resulting plate scale of the telescope + CCD system is about 1.2 arc seconds per pixel, the exposure used was 10 seconds per frame, short enough to prevent the asteroid drift.
This case highlights the different classification scheme used by different organitazions. Having a semimajor axis a = 1.533 and perihelion distance q = 1.005, 2010 NG is Amor for the MPC and Apollo for the JPL.
The MPC NEO classes :
Atens have semimajor axes, a, less than 1 AU;
Apollos have semimajor axes, a, greater than 1 AU, and perihelion distances, q, less than 1 AU;
Amors have perihelion distances between 1 and 1.3 AU.
The JPL Orbits classes :
Aten Near-Earth asteroid orbits similar to that of 2062 Aten (a < 1.0 AU; Q > 0.983 AU).
Apollo Near-Earth asteroid orbits which cross the Earth's orbit similar to that of 1862 Apollo (a > 1.0 AU; q < 1.017 AU).
Amor Near-Earth asteroid orbits similar to that of 1221 Amor (a > 1.0 AU; 1.017 < q < 1.3 AU).
Reference : MPEC 2010-N15
This case highlights the different classification scheme used by different organitazions. Having a semimajor axis a = 1.533 and perihelion distance q = 1.005, 2010 NG is Amor for the MPC and Apollo for the JPL.
The MPC NEO classes :
Atens have semimajor axes, a, less than 1 AU;
Apollos have semimajor axes, a, greater than 1 AU, and perihelion distances, q, less than 1 AU;
Amors have perihelion distances between 1 and 1.3 AU.
The JPL Orbits classes :
Aten Near-Earth asteroid orbits similar to that of 2062 Aten (a < 1.0 AU; Q > 0.983 AU).
Apollo Near-Earth asteroid orbits which cross the Earth's orbit similar to that of 1862 Apollo (a > 1.0 AU; q < 1.017 AU).
Amor Near-Earth asteroid orbits similar to that of 1221 Amor (a > 1.0 AU; 1.017 < q < 1.3 AU).
Reference : MPEC 2010-N15
Monday, June 7, 2010
2010 June 06, NEO confirmations
The night of the Sunday 06 june 2010, working remotely from Madrid, I contributed to the confirmation of two objects posted on the MPC's NEO confirmation page (NEOCP), one of them (TAL 601) was moving quite fast, at about 4"/sec, allowing only short exposures max 20 seconds :
TAL 601 = 2010 LN14 Apollo object
Reference : MPEC 2010-L30
SW40jD = 2010 LJ14 This is an amor object, it grazes the Earth's orbit at a periheion of 1.1 AU, see the orbit diagram at JPL orbits
Reference : MPEC 2010-L27
Also, previous confirmation work, conducted on the site on June 5 and 4 :
RL2C068 = 2010 CL17 This resulted to be a a main belt asteroid.
RL2B422 According to the MPC this was not a minor planet, however I didn't find any object around the predicted position, also strange how this object didn't have uncertainty map pusblished in the NEOCP as usual.
TAL 601 = 2010 LN14 Apollo object
Reference : MPEC 2010-L30
SW40jD = 2010 LJ14 This is an amor object, it grazes the Earth's orbit at a periheion of 1.1 AU, see the orbit diagram at JPL orbits
Reference : MPEC 2010-L27
Also, previous confirmation work, conducted on the site on June 5 and 4 :
RL2C068 = 2010 CL17 This resulted to be a a main belt asteroid.
RL2B422 According to the MPC this was not a minor planet, however I didn't find any object around the predicted position, also strange how this object didn't have uncertainty map pusblished in the NEOCP as usual.
Subscribe to:
Comments (Atom)