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Sky-Tonight.com / Asteroids / 179 Klytaemnestra
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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 Klytaemnestra Observation Details

Klytaemnestra

Klytaemnestra Daily Motion


179 Klytaemnestra will become visible in August, 5. After being too close to the Sun to observe, it will reappear in the night sky. Starting from August, 5, 179 Klytaemnestra can be seen again, providing a good opportunity for observation.

Klytaemnestra Visibility on June 14

179 Klytaemnestra rises at sunrise

Klytaemnestra Rise and Set Timetable

TimeElevation
Moon Rise, 7% illuminated 01:59-6°
Klytaemnestra transit09:4975°
Klytaemnestra set17:01
Moon Set17:31-5°
Astrosession begin20:22-27°
Astrosession end01:53-7°
Klytaemnestra rise02:34
Twighlight end02:361°
Civil sunrise03:158°
Sunrise03:4814°

Track Klytaemnestra Position Throughout the Night

← Sun, 14 June 2026 →

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

Klytaemnestra Description

Klytaemnestra, designated as 179 Klytaemnestra, is a main-belt asteroid, located between Mars and Jupiter in the solar system. With a diameter of 70 km, 179 Klytaemnestra completes its orbit around the Sun in 5.1 years. At the moment, 179 Klytaemnestra is 3.741 AU (559,645,634 km) from Earth, and it is located in the constellation Taurus.

Current position of Klytaemnestra in Solar System

Earth Klytaemnestra
DateSun, 14 June 2026
Distance from Earth to Klytaemnestra3.74 AU (559,496,036km)
Elongation18°
Angular diameter"
Magnitude13.85
This interactive projection shows the current positions of Klytaemnestra, Earth, and the Sun in the Solar System. By sliding the image left or right, you can change the day of the year and see how Klytaemnestra and Earth move along their orbits around the Sun.

Finder Chart for Klytaemnestra

Double-click to unlock the map.
Object name179 Klytaemnestra
Field of view
Limiting magnitude
179 Klytaemnestra coordinates4.1552014256468, 22.414599855941
Center coordinates4.1552014256468, 22.414599855941

Annual motion of Klytaemnestra

Time
DateSun, 14 June 2026
Twighlight start20:17
Twighlight end01:47
Twighlight duration5h 30m
Rise02:34
Set16:58
Elevation at transit75°
Transit time09:46
Equatorial coordinatesRA: 04h 11m 02s", Dec: 22° 28' 09s
Magnitude14
ConstellationTaurus
The graph illustrates the annual visibility pattern of a Klytaemnestra, 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 Klytaemnestra 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. You can also view detailed visibility information in a dedicated table, including exact rise, transit, and set times for each date.

Astrometric & Physical Parameters of 179 Klytaemnestra

Coordinates & Visibility

Right Ascension4.1552014256468°
Declination22.414599855941°
Magnitude13.85
ConstellationTaurus
Elevation53.1°
Azimuth102.6°

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.