Asteroid Pallas Observation Details
Pallas Daily Motion
2 Pallas will be visible until February, 11, 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 on June 29
2 Pallas is visible in the early morning sky until sunrise
Pallas Rise and Set Timetable
| Time | Elevation | |
Moon Rise, 98.9% illuminated  | 18:05 | -49° |
| Astrosession begin | 20:25 | -35° |
| Pallas rise | 23:34 | |
| Astrosession end | 01:56 | 28° |
| Twighlight end | 02:40 | 36° |
| Moon Set | 03:13 | 42° |
| Civil sunrise | 03:19 | 43° |
| Sunrise | 03:51 | 47° |
| Pallas transit | 05:44 | 56° |
Track Pallas Position Throughout the Night
← Mon, 29 June 2026 →
| 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 3.026 AU (452,683,157 km) from Earth, and it is located in the constellation Pisces.Current position of Pallas in Solar System
| Date | Mon, 29 June 2026 |
| Distance from Earth to Pallas | 3.026 AU (452,683,157km) |
| Elongation | 80° |
| Angular diameter | " |
| Magnitude | 9.95 |
Finder Chart for Pallas
Double-click to unlock the map.
| Object name | 2 Pallas |
| Field of view | |
| Limiting magnitude | |
| 2 Pallas coordinates | 1.1277523291718, 3.6339147661126 |
| Center coordinates | 1.1277523291718, 3.6339147661126 |
Annual motion of Pallas
| Date | Tue, 30 June 2026 |
| Twighlight start | 20:24 |
| Twighlight end | 01:55 |
| Twighlight duration | 6h 31m |
| Rise | 23:31 |
| Set | 11:51 |
| Elevation at transit | 56° |
| Transit time | 05:41 |
| Equatorial coordinates | RA: 01h 08m 35s", Dec: 03° 36' 16s |
| Magnitude | 10 |
| Constellation | Pisces |
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. You can also view detailed visibility information in a dedicated table, including exact rise, transit, and set times for each date.
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. 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 2 Pallas
Coordinates & Visibility
| Right Ascension | 1.1277523291718° |
| Declination | 3.6339147661126° |
| Magnitude | 9.95 |
| Constellation | Pisces |
| Elevation | -11.9° |
| Azimuth | -76° |
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.