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Sky-Tonight.com / Asteroids / 18 Melpomene
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Observation Settings

Or select it on the map:
This Earth map fragment is intended to illustrate celestial motion across the sky, emphasizing both bearing and elevational perspectives. The map's center point corresponds to the transit, showcasing celestial objects at their highest point, while elevation gradually decreases towards the map edges. This dynamic representation offers insights into the changing positions of celestial bodies with a focus on their bearing and elevational trajectories.
Your location: Santa Clara, United States
Timezone:
Latitude:
37.3541
Longitude:
-121.955

Asteroid 18 Melpomene Observation Details

Melpomene

Melpomene Daily Motion

Tonight, observing Melpomene may prove challenging owing to its low elevation. It will reach its transit at by 08:30 and set before sunset at 13:47. Rising near twilight's end at 03:12, it will fade away by 03:44, peaking at just 6° above the horizon.
18 Melpomene will become visible in February, 23. After being too close to the Sun to observe, it will reappear in the night sky. Starting from February, 23, 18 Melpomene can be seen again, providing a good opportunity for observation.

Melpomene Visibility Timetable on December 20

Melpomene Rise and Set Timetable

TimeElevation
Moon Rise, 0.4% illuminated05:1922°
Melpomene transit08:3039°
Melpomene set13:47
Moon Set14:25-7°
Astrosession begin16:26-31°
Melpomene rise03:12
Astrosession end03:446°
Civil sunrise04:4818°
Sunrise05:1922°

Track Melpomene Position Throughout the Night

← Sat, 20 December 2025 →

Elevation (degrees)
Time
Altitude
Azimuth
Shift the map to change the time and observe Melpomene changing position in the night sky.

Melpomene Description

Melpomene, designated as 18 Melpomene, is a main-belt asteroid, located between Mars and Jupiter in the solar system. With a diameter of 140 km, 18 Melpomene completes its orbit around the Sun in 3.5 years. At the moment, 18 Melpomene is 3.502 AU (523,891,743 km) from Earth, and it is located in the constellation Scorpius.

Current position of Melpomene in Solar System

Earth Melpomene
DateSat, 20 December 2025
Distance from Earth to Melpomene3.502 AU (523,891,743km)
Elongation25°
Angular diameter"
Magnitude11.71
This section provides an interactive projection of the solar system, illustrating the relative positions of Melpomene, Earth, and the Sun throughout the year. By sliding the image left or right, you can change the day of the year, observing how the positions of Melpomene and Earth shift in their orbits around the Sun.

Finder Chart for Melpomene

Double-click to unlock the map.
Object name18 Melpomene
Field of view
Limiting magnitude
18 Melpomene coordinates16.29860155269, -13.64899753139
Center coordinates16.29860155269, -13.64899753139

Annual motion of Melpomene

Time
DateSun, 21 December 2025
Twighlight start16:22
Twighlight end03:38
Twighlight duration11h 16m
Rise03:08
Set13:41
Elevation at transit39°
Transit time08:25
Equatorial coordinatesRA: 16h 19m 38s", Dec: -13° 42' 30s
Magnitude12
ConstellationScorpius
The graph illustrates the annual visibility pattern of a Melpomene, providing a comprehensive overview of its daily appearances and transit times throughout the year.
The graph is structured with the vertical axis showing the hours of the day, ranging from 12 AM to 12 AM the next day, while the horizontal axis spans each day of the year.
The reddish shaded area indicates the periods when the Melpomene is above the horizon, visible to observers. The white line marks the times when the celestial object reaches its highest point in the sky each day, known as the transit.

Astrometric & Physical Parameters of 18 Melpomene

Coordinates & Visibility

Right Ascension16.29860155269°
Declination-13.64899753139°
Magnitude11.71
ConstellationScorpius
Elevation-24.3°
Azimuth-88.9°

Acknowledgments

We acknowledge NASA's Jet Propulsion Laboratory (JPL) for providing essential data on asteroids and comets through their Small-Body Database (SBDB) and Center for Near-Earth Object Studies (CNEOS). Their continuous efforts in tracking and cataloging these celestial bodies make it possible to offer accurate and up-to-date information on their positions, orbits, and physical characteristics.