Comet 90004801 C/2023 R2 (PANSTARRS) Observation Details
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C/2023 R2 (PANSTARRS) Daily Motion
C/2023 R2 (PANSTARRS) is circumpolar, never setting below the horizon and always visible in the night sky from your location. However, it will change its position significantly, moving 54 degrees over time. You can find the best times to observe C/2023 R2 (PANSTARRS), when it reaches its highest elevation, in the annual motion section.90004801 C/2023 R2 (PANSTARRS) will be visible until March, 7, 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.
C/2023 R2 (PANSTARRS) Visibility Timetable on September 03
C/2023 R2 (PANSTARRS) Rise and Set Timetable
Time | Elevation | |
C/2023 R2 (PANSTARRS) is always above the horizon | ||
C/2023 R2 (PANSTARRS) transit | 12:56 | 64° |
Moon Rise, 75.5% illuminated | 14:44 | 60° |
Sunset | 17:33 | 42° |
Civil sunset | 18:01 | 39° |
Astrosession begin | 19:05 | 32° |
C/2023 R2 (PANSTARRS) is always above the horizon | ||
Moon Set | 23:57 | 11° |
Astrosession end | 03:09 | 14° |
Civil sunrise | 04:13 | 18° |
Sunrise | 04:41 | 20° |
Track C/2023 R2 (PANSTARRS) Position Throughout the Night
← Wed, 3 September 2025 →
Time | |
Altitude | |
Azimuth |
Shift the map to change the time and observe C/2023 R2 (PANSTARRS) changing position in the night sky.
C/2023 R2 (PANSTARRS) Description
C/2023 R2 (PANSTARRS), designated as 90004801 C/2023 R2 (PANSTARRS), is a comet on a hyperbolic (unbound) trajectory. At the moment, 90004801 C/2023 R2 (PANSTARRS) is 4.781 AU (715,212,460 km) from Earth, and it is located in the constellation Ursa Major.Current position of C/2023 R2 (PANSTARRS) in Solar System
Date | Wed, 3 September 2025 |
Distance from Earth to C/2023 R2 (PANSTARRS) | 4.7809 AU (715,212,460km) |
Elongation | 59° |
Angular diameter | " |
Magnitude | 16.9 |
Finder Chart for C/2023 R2 (PANSTARRS)
Double-click to unlock the map.
Object name | 90004801 C/2023 R2 (PANSTARRS) |
Field of view | |
Limiting magnitude | |
90004801 C/2023 R2 (PANSTARRS) coordinates | 12.63797, 62.923 |
Center coordinates | 12.63797, 62.923 |
Annual motion of C/2023 R2 (PANSTARRS)
Date | Thu, 4 September 2025 |
Twighlight start | 19:03 |
Twighlight end | 03:08 |
Twighlight duration | 8h 5m |
Rise | 90004801 C/2023 R2 (PANSTARRS) is always up |
Set | 90004801 C/2023 R2 (PANSTARRS) is always up |
Elevation at transit | 64° |
Transit time | 12:55 |
Equatorial coordinates | RA: 12h 40m 24s", Dec: 62° 55' 19s |
Magnitude | 17 |
Constellation | Ursa Major |
The graph illustrates the annual visibility pattern of a C/2023 R2 (PANSTARRS), 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 C/2023 R2 (PANSTARRS) 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 C/2023 R2 (PANSTARRS) 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 90004801 C/2023 R2 (PANSTARRS)
Coordinates & Visibility
Right Ascension | 12.63797° |
Declination | 62.923° |
Magnitude | 16.9 |
Constellation | Ursa Major |
Elevation | 17.4° |
Azimuth | 20.9° |
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.