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© NASA/Galileo 1993. Pictured asteroid is 243 Ida.

Asteroid 9 Metis at opposition

Tue, 01 Jan 2013 at08:08 EST(142 days ago)
13:08 UTC

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Asteroid 9 Metis will be well placed for observation, lying in the constellation Gemini, well above the horizon for much of the night. Regardless of your location, Metis will reach its highest point in the sky at around midnight, local time, an optimal positioning that occurs when it makes its closest approach to the point in the sky directly opposite to the Sun – an event termed opposition, the exact moment of which will be 08:08 UTC. 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 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 Metis lies opposite to the Sun in the night sky, the Solar System is lined up so that 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 Metis. On this occasion, Metis will pass within 1.138 AU of us, reaching a peak brightness of magnitude 8.2. Nonetheless, even at its brightest, Metis is a faint object beyond the reach of the naked eye or binoculars; a telescope of moderate aperture and a good star chart are needed.

At the moment of opposition, Metis will lie at a declination of +28°30' , and so will be seen to best advantage in the northern hemisphere; in fact, it will be unobservable from latitudes much south of 41°S.

The finder chart and ephemeris below indicate the path of Metis around the time of its opposition; the ephemeris also provides estimates of the asteroid's apparent magnitude.

Light-on-dark | Dark-on-light | 3D orbit view

The exact position of Metis at the moment of opposition are as follows:

Object Right Ascension Declination Constellation Magnitude
Asteroid 9 Metis 06h51m24s +28°30'07" Gemini 8.2

The coordinates above are given in J2000.0.

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The following ephemeris describes the movement of Metis in the weeks around its opposition:

|     DATE     | RIGHT ASCENS | DECLINATION | approx| phase | solar  | CONSTELLATION
| Year Mth Day | hour min sec | deg min sec | mag.  |       |distance|
|                                                     (0-1)  (deg)   |
|
| 2012  10  22 |   07  02  40 | +23  41  36 |  8.98 | 0.944 | 104.99 | Gemini
| 2012  11  01 |   07  11  27 | +23  59  56 |  8.82 | 0.950 | 113.00 | Gemini
| 2012  11  08 |   07  15  49 | +24  17  19 |  8.71 | 0.955 | 119.06 | Gemini
| 2012  11  15 |   07  18  30 | +24  39  19 |  8.61 | 0.962 | 125.52 | Gemini
| 2012  11  22 |   07  19  23 | +25  06  16 |  8.50 | 0.969 | 132.42 | Gemini
| 2012  12  01 |   07  17  44 | +25  47  50 |  8.38 | 0.979 | 141.92 | Gemini
| 2012  12  08 |   07  14  17 | +26  24  27 |  8.30 | 0.986 | 149.76 | Gemini
| 2012  12  15 |   07  09  05 | +27  03  00 |  8.24 | 0.992 | 157.92 | Gemini
| 2012  12  22 |   07  02  26 | +27  41  07 |  8.20 | 0.997 | 166.12 | Gemini
| 2013  01  01 |   06  51  28 | +28  29  55 |  8.19 | 1.000 | 174.43 | Gemini
| 2013  01  08 |   06  43  35 | +28  57  23 |  8.22 | 0.998 | 169.58 | Gemini
| 2013  01  15 |   06  36  18 | +29  18  03 |  8.27 | 0.995 | 161.61 | Auriga
| 2013  01  22 |   06  30  11 | +29  31  49 |  8.35 | 0.989 | 153.45 | Auriga
| 2013  02  01 |   06  24  18 | +29  41  09 |  8.48 | 0.980 | 142.24 | Auriga
| 2013  02  08 |   06  22  27 | +29  41  54 |  8.60 | 0.973 | 134.84 | Auriga
| 2013  02  15 |   06  22  32 | +29  39  02 |  8.71 | 0.966 | 127.87 | Auriga
| 2013  02  22 |   06  24  30 | +29  33  16 |  8.84 | 0.960 | 121.31 | Auriga
| 2013  03  01 |   06  28  12 | +29  25  06 |  8.96 | 0.955 | 115.14 | Auriga
| 2013  03  08 |   06  33  27 | +29  14  38 |  9.08 | 0.951 | 109.33 | Auriga
| 2013  03  15 |   06  40  05 | +29  01  49 |  9.20 | 0.948 | 103.84 | Gemini
|
| Ephemeris computed by Dominic Ford, 03 April 2013.


Source
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.

Image credit
© NASA/Galileo 1993. Pictured asteroid is 243 Ida.