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Ephemeris

              Right                   Distance    From 47N 7E:
            Ascension    Declination      (AU)   Altitude Azimuth
Sun         22h 47m 56s    -7 38.1'     0.991    31.233   28.579 Up
Mercury       21h 4m 4s    -17 1.2'     0.955    11.661   48.734 Up
Venus         20h 1m 9s   -19 29.6'     1.023     0.959   59.516 Up
Moon        22h 44m 32s    -3 26.3'   60.3 ER    34.889   31.240 Up
Mars         9h 21m 36s   +19 55.0'     0.711   -11.337 -136.424 Set
Jupiter     16h 50m 39s   -21 41.0'     5.333   -31.661   91.422 Set
Saturn       23h 5m 28s    -7 44.5'    10.653    32.449   23.668 Up
Uranus       20h 4m 13s   -20 53.5'    20.430     0.309   58.083 Up
Neptune     19h 45m 59s   -20 39.0'    30.855    -2.189   61.544 Set
Pluto        16h 5m 24s    -6 54.3'    29.643   -28.449  112.365 Set
1995 DW1     12h 3m 42s    +2 55.2'     0.451   -39.852 -172.924 Set

The ephemeris shows you the positions of the principal bodies in the Solar System at the selected time, both in celestial coordinates and as seen from your specified observing site. If you're tracking an asteroid or comet by specifying its orbital elements, its position is given at the foot of the table. The sample ephemeris above gives positions for 13:31:56 UTC on March 1, 1995, while tracking the Earth-orbit-crossing asteroid 1995 DW1, whose discovery (on February 25, 1995) was reported in Minor Planet Electronic Circular 1995-E02 of 00:15 UTC, March 1, 1995, giving the orbital elements shown at the end of this page.

For each solar system body the following data are displayed: The first three items give the equatorial celestial coordinates of the object at the specified time, and its distance from the Earth. These values are independent of the observing site.

Right ascension
Hour angle at Greenwich.
Declination
Declination with regard to the equator.
Distance (AU)
Distance from the Earth in astronomical units (the Moon's distance is given in units of the Earth's radius).

The next three columns give the location of the object in the sky at the specified observing site.

Altitude
Altitude of the body above the horizon, in degrees at the observing site. If negative, the body is below the horizon (“set”) and hence invisible.
Azimuth
Local compass bearing to the object at the observing site. Astronomers measure azimuth from the South (consistent with the convention for hour angle), with positive angles toward the West and negative angles toward the East.
Visibility
This column interprets the Altitude and Azimuth to describe what you can expect to see. Objects below the apparent horizon (taking account of the refraction of the atmosphere and the finite angular size of the Sun and Moon but not altitude of the observer) are shown as “Set” while objects clearly visible in the sky (or visible if the Sun weren't also up) are shown as “Up”. Objects that are just appearing or disappearing on the horizon are shown as “Rising” or “Setting”, and objects at culmination (crossing the local meridian) are shown as being in “Transit”. Transit times are quite accurate, but rising and setting times can be given only approximately because the altitude of the observer, local topography along the horizon, and the effects of atmospheric refraction (which, in turn, vary based upon temperature and barometric pressure) have a major influence upon when you will actually see an object appear or disappear at the horizon.

Press the button to reproduce the sample ephemeris above, using the following orbital elements for asteroid 1995 DW1:

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