Dominic Ford, Editor
From the Asteroids feed
Asteroid 12 Victoria will be well placed for observation, lying in the constellation Pegasus, well above the horizon for much of the night.
Regardless of your location on the Earth, 12 Victoria will reach its highest point in the sky around midnight local time.
From Cambridge, it will be visible in the evening sky, becoming accessible around 20:14 (EST) as the dusk sky fades, 28° above your eastern horizon. It will then reach its highest point in the sky at 00:13, 57° above your southern horizon. It will continue to be observable until around 04:48, when it sinks below 22° above your western horizon.
The geometry of the alignment
This optimal positioning occurs when it makes its closest approach to the point in the sky directly opposite to the Sun – an event termed opposition. Since the Sun reaches its greatest distance below the horizon at midnight, the point opposite to it is highest in the sky at the same time.
At around the same time that 12 Victoria passes opposition, it also makes its closest approach to the Earth – termed its perigee – making it appear at its brightest in the night sky. This happens because when 12 Victoria lies opposite to the Sun in the night sky, the solar system is lined up so that 12 Victoria, the Earth and the Sun lie in a straight line with the Earth in the middle, on the same side of the Sun as 12 Victoria.
On this occasion, 12 Victoria will pass within 0.912 AU of us, reaching a peak brightness of magnitude 9.0. Nonetheless, even at its brightest, 12 Victoria is a faint object beyond the reach of the naked eye; binoculars or a telescope of moderate aperture are needed.
Finding 12 Victoria
The chart below indicates the path of 12 Victoria across the sky around the time of opposition.
The position of 12 Victoria at the moment of opposition will be as follows:
|Asteroid 12 Victoria||22h40m30s||+09°32'||Pegasus||9.0|
The coordinates above are given in J2000.0.
|The sky on 09 September 2014|
15 days old
All times shown in EDT.
The circumstances of this event were computed from orbital elements made available by Ted Bowell of the Lowell Observatory. The conversion to geocentric coordinates was performed using the position of the Earth recorded in the DE405 ephemeris published by the Jet Propulsion Laboratory (JPL).
The star chart above shows the positions and magnitudes of stars as they appear in the Tycho catalogue. The data was reduced by the author and plotted using PyXPlot. A gnomonic projection of the sky has been used; celestial coordinates are indicated in the J2000.0 coordinate system.