Asteroid 2 Pallas Observation Details
Pallas Daily Motion
Pallas will rise at 12:04, reaching 56° when twilight begins at 18:07. It will reach transit at 56° by 18:12 and will set before twilight ends at 00:21.2 Pallas will be visible until December, 31, 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.
Pallas Visibility Timetable on October 08
Pallas Rise and Set Timetable
| Time | Elevation | |
| Pallas rise | 12:04 | |
| Sunset | 16:40 | 50° |
| Moon Rise, 98.7% illuminated | 16:55 | 51° |
| Civil sunset | 17:07 | 52° |
| Astrosession begin | 18:07 | 56° |
| Pallas transit | 18:12 | 56° |
| Pallas set | 00:21 | |
| Astrosession end | 03:43 | -37° |
| Moon Set | 07:05 | -48° |
Track Pallas Position Throughout the Night
← Wed, 8 October 2025 →
| Time | |
| Altitude | |
| Azimuth |
Shift the map to change the time and observe Pallas changing position in the night sky.
Pallas Description
Pallas, designated as 2 Pallas, is a main-belt asteroid, located between Mars and Jupiter in the solar system. With a diameter of 514 km, 2 Pallas completes its orbit around the Sun in 4.6 years. At the moment, 2 Pallas is 2.901 AU (433,983,423 km) from Earth, and it is located in the constellation Aquila.Current position of Pallas in Solar System
| Date | Wed, 8 October 2025 |
| Distance from Earth to Pallas | 2.903 AU (434,282,619km) |
| Elongation | 110° |
| Angular diameter | " |
| Magnitude | 9.99 |
Finder Chart for Pallas
Double-click to unlock the map.
| Object name | 2 Pallas |
| Field of view | |
| Limiting magnitude | |
| 2 Pallas coordinates | 20.218949871877, 3.0183660656621 |
| Center coordinates | 20.218949871877, 3.0183660656621 |
Annual motion of Pallas
| Date | Wed, 8 October 2025 |
| Twighlight start | 18:03 |
| Twighlight end | 03:36 |
| Twighlight duration | 10h 33m |
| Rise | 12:01 |
| Set | 00:16 |
| Elevation at transit | 55° |
| Transit time | 18:09 |
| Equatorial coordinates | RA: 20h 13m 23s", Dec: 02° 50' 37s |
| Magnitude | 10 |
| Constellation | Aquila |
The graph illustrates the annual visibility pattern of a Pallas, 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 Pallas 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.
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 Pallas 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 2 Pallas
Coordinates & Visibility
| Right Ascension | 20.218949871877° |
| Declination | 3.0183660656621° |
| Magnitude | 9.98 |
| Constellation | Aquila |
| Elevation | -1° |
| Azimuth | -85.4° |
Physical properties
| Mean radius in kilometres | 545 |
| Boby mass in kg | 2.11E+20 |
| Body density in g.cm3 | 1 |
Orbital Parameters
| Sideral orbital time for body around another one (the Sun or a planet) in earth day | 1685.927 |
Data Acknowledgment
Our solar system data—including planetary physical and orbital parameters—comes from the Solar System OpenData API , maintained by Le Système Solaire. We thank Christophe and the contributors for making this open data available.
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.