151.205000,-33.861527,0.0751113 {E-lon(deg),Lat(deg),Alt(km)}
HTML Code:
Date__(UT)__HR:MN R.A._(ICRF/J2000.0)_DEC Azi_(a-appr)_Elev APmag Illu% Cnst
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2013-Feb-15 12:00 00 44 29.88 -82 50 26.5 188.1776 31.6310 13.76 34.736 Oct
2013-Feb-15 13:00 01 03 07.96 -84 11 55.0 186.1517 31.1171 13.39 35.844 Oct
2013-Feb-15 14:00 01 55 36.92 -85 57 12.2 184.2508 31.8335 12.94 37.470 Oct
2013-Feb-15 15:00 05 16 22.91 -87 21 50.2 183.1775 34.0851 12.38 39.958 Oct
2013-Feb-15 16:00 09 21 22.25 -84 20 13.3 184.2858 38.2683 11.65 43.998 Oct
2013-Feb-15 17:00 10 30 01.66 -76 02 30.0 191.0498 44.8470 10.65 51.162 Cha
2013-Feb-15 18:00 10 56 35.42 -58 44 08.2 215.2169 52.3851 9.25 65.249 Car
Times are UTC.
Sydney is UTC + 11 hours.
So, for example, 2013-Feb-15 12:00 UTC corresponds to 2013-Feb-15 23:00 AEDT,
that is 11pm in Sydney on the night of the 15th of Feb.
R.A._(ICRF/J2000.0)_DEC =
J2000.0 astrometric right ascension and declination of target center.
Azi_(a-appr)_Elev =
Airless apparent azimuth and elevation of target center. Corrected for
light-time, the gravitational deflection of light, stellar aberration,
precession and nutation. Azimuth measured North(0) -> East(90) -> South(180) ->
West(270) -> North (360). Elevation is with respect to plane perpendicular
to local zenith direction. TOPOCENTRIC ONLY. Units: DEGREES
APmag =
Asteroid's approximate apparent visual magnitude by following definition:
APmag = H + 5*log10(delta) + 5*log10(r) - 2.5*log10((1-G)*phi1 + G*phi2).
In principle, accurate to ~ +/- 0.1 magnitude. For solar phase angles > 90 deg,
the error could exceed 1 magnitude. No values are output for phase angles
greater than 120 degrees, since the extrapolation error could be large and
unknown. Units: NONE
Illu% =
Fraction of target circular disk illuminated by Sun (phase), as seen by
observer. Units: PERCENT
Cnst =
Constellation ID; the 3-letter abbreviation for the name of the
constellation containing the target center's astrometric position,
as defined by IAU (1930) boundary delineation.