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Sky-Tonight.com / Asteroids / 82 Alkmene
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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 82 Alkmene Observation Details

Alkmene

Alkmene Daily Motion

Alkmene will be visible throughout the entire night. It will rise at 14:29, just before twilight begins, and will be at 23° when twilight starts at 16:40. It will reach its transit at 80° at 22:01, and will fade away as twilight ends at 03:49, being at 18° elevation.
82 Alkmene will be visible until June, 9, when it will move too close to the Sun. During this time, its proximity to the Sun will cause it to disappear from the night sky, making it unobservable for a while.

Alkmene Visibility Timetable on January 10

Alkmene Rise and Set Timetable

TimeElevation
Alkmene rise14:29
Sunset15:066°
Civil sunset15:3612°
Astrosession begin16:4023°
Alkmene transit22:0180°
Moon Rise, 53.2% illuminated22:1380°
Astrosession end03:4918°
Civil sunrise04:537°
Sunrise05:232°
Alkmene set05:33
Moon Set09:26-25°

Track Alkmene Position Throughout the Night

← Sat, 10 January 2026 →

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

Alkmene Description

Alkmene, designated as 82 Alkmene, is a main-belt asteroid, located between Mars and Jupiter in the solar system. With a diameter of 58 km, 82 Alkmene completes its orbit around the Sun in 4.6 years. At the moment, 82 Alkmene is 1.221 AU (182,659,000 km) from Earth, and it is located in the constellation Gemini.

Current position of Alkmene in Solar System

Earth Alkmene
DateSat, 10 January 2026
Distance from Earth to Alkmene1.221 AU (182,659,000km)
Elongation174°
Angular diameter"
Magnitude10.65
This section provides an interactive projection of the solar system, illustrating the relative positions of Alkmene, 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 Alkmene and Earth shift in their orbits around the Sun.

Finder Chart for Alkmene

Double-click to unlock the map.
Object name82 Alkmene
Field of view
Limiting magnitude
82 Alkmene coordinates7.2190969196737, 27.466946367471
Center coordinates7.2190969196737, 27.466946367471

Annual motion of Alkmene

Time
DateSun, 11 January 2026
Twighlight start16:41
Twighlight end03:47
Twighlight duration11h 6m
Rise14:24
Set05:28
Elevation at transit80°
Transit time21:56
Equatorial coordinatesRA: 07h 12m 08s", Dec: 27° 29' 52s
Magnitude11
ConstellationGemini
The graph illustrates the annual visibility pattern of a Alkmene, 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 Alkmene 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 82 Alkmene

Coordinates & Visibility

Right Ascension7.2190969196737°
Declination27.466946367471°
Magnitude10.65
ConstellationGemini
Elevation15.4°
Azimuth-66.9°

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.