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
