Asteroid 444 Gyptis Observation Details

Gyptis Daily Motion
Gyptis will rise at 02:13, during twilight, and will ascend to 23° by the time twilight ends at 04:13.444 Gyptis will be visible until March, 5, 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.
Gyptis Visibility Timetable on May 25
Gyptis Rise and Set Timetable
Time | Elevation | |
Moon Rise, 11.4% illuminated | 04:09 | 21° |
Moon Set | 18:12 | -38° |
Astrosession begin | 22:44 | -37° |
Gyptis rise | 02:13 | |
Astrosession end | 04:13 | 23° |
Civil sunrise | 05:37 | 37° |
Sunrise | 06:10 | 42° |
Gyptis transit | 08:22 | 53° |
Track Gyptis Position Throughout the Night
← Sun, 25 May 2025 →
Time | |
Altitude | |
Azimuth |
Shift the map to change the time and observe Gyptis changing position in the night sky.
Gyptis Description
Gyptis, designated as 444 Gyptis, is a main-belt asteroid, located between Mars and Jupiter in the solar system. With a diameter of 160 km, 444 Gyptis completes its orbit around the Sun in 4.6 years. At the moment, 444 Gyptis is 2.366 AU (353,948,562 km) from Earth, and it is located in the constellation Pisces.Current position of Gyptis in Solar System
Date | Sun, 25 May 2025 |
Distance from Earth to Gyptis | 2.36 AU (353,050,975km) |
Elongation | 76° |
Angular diameter | " |
Magnitude | 12.83 |
Finder Chart for Gyptis
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Object name | 444 Gyptis |
Field of view | |
Limiting magnitude | |
444 Gyptis coordinates | 23.044630171709, 2.6584000695002 |
Center coordinates | 23.044630171709, 2.6584000695002 |
Annual motion of Gyptis
Date | Sun, 25 May 2025 |
Twighlight start | 22:39 |
Twighlight end | 04:08 |
Twighlight duration | 5h 29m |
Rise | 02:14 |
Set | 14:31 |
Elevation at transit | 53° |
Transit time | 08:22 |
Equatorial coordinates | RA: 23h 04m 03s", Dec: 02° 48' 40s |
Magnitude | 13 |
Constellation | Pisces |
The graph illustrates the annual visibility pattern of a Gyptis, 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 Gyptis 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 Gyptis 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.
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.