Dominic Ford, Editor
From the Asteroids feed
Asteroid 9 Metis will be well placed for observation, lying in the constellation Leo, well above the horizon for much of the night.
Regardless of your location on the Earth, 9 Metis will reach its highest point in the sky around midnight local time.
From Cambridge, it will be visible in the morning sky, becoming accessible around 18:51, when it rises to an altitude of 21° above your eastern horizon. It will then reach its highest point in the sky at 00:14, 69° above your southern horizon. It will be lost to dawn twilight around 05:34, 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 9 Metis 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 9 Metis lies opposite to the Sun in the night sky, the solar system is lined up so that 9 Metis, the Earth and the Sun lie in a straight line with the Earth in the middle, on the same side of the Sun as 9 Metis.
On this occasion, 9 Metis will pass within 1.277 AU of us, reaching a peak brightness of magnitude 8.9. Nonetheless, even at its brightest, 9 Metis is a faint object beyond the reach of the naked eye; binoculars or a telescope of moderate aperture are needed.
Finding 9 Metis
The chart below indicates the path of 9 Metis across the sky around the time of opposition.
The position of 9 Metis at the moment of opposition will be as follows:
|Asteroid 9 Metis||10h05m10s||+21°59'||Leo||8.9|
The coordinates above are given in J2000.0.
|The sky on 14 February 2028|
19 days old
All times shown in EST.
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.