Double Star 10435+4612 Observation Details
10435+4612 Daily Motion
10435+4612 will reach its transit before twilight, at 20:23. By the onset of twilight at 21:54, it will be at 72° elevation, and it will set before after, at 06:25.10435+4612 will be visible until July, 21, 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.
10435+4612 Visibility Timetable on May 20
10435+4612 Rise and Set Timetable
| Time | Elevation | |
| 10435+4612 transit | 20:23 | 84° |
| Sunset | 20:42 | 83° |
| Civil sunset | 21:15 | 79° |
| Astrosession begin | 22:37 | 65° |
| Moon Rise, 52.6% illuminated | 02:29 | 27° |
| Astrosession end | 04:19 | 12° |
| Civil sunrise | 05:41 | 3° |
| Sunrise | 06:13 | 1° |
| 10435+4612 set | 06:25 | |
| 10435+4612 rise | 10:17 | |
| Moon Set | 13:16 | 18° |
Track 10435+4612 Position Throughout the Night
← Tue, 20 May 2025 →
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Shift the map to change the time and observe 10435+4612 changing position in the night sky.
10435+4612 Star System Description
10435+4612 is 8-star Star System located in constellation Ursa Major at coordinates RA: 10h 43m 32s", Dec: 46° 12' 13s.
The primary component has a magnitude of 5.21, while the secondary component has a magnitude of 7.35. They are separated by 4.8 arcminutes at a position angle of 88 degrees. The brightness difference between the two components is 2.14 magnitudes, with the primary component being approximately 7.2 times brighter than the secondary.
Below is a table with star system details from the Washington Double Star (WDS) Catalog. This catalog is a comprehensive source of information on double and multiple star systems, providing key data on the positions, magnitudes, and separations of stellar components.
T: Statistically the same parallax within the errors and similar proper motion or other technique indicates that this pair is physical.
The primary component has a magnitude of 5.21, while the secondary component has a magnitude of 7.35. They are separated by 4.8 arcminutes at a position angle of 88 degrees. The brightness difference between the two components is 2.14 magnitudes, with the primary component being approximately 7.2 times brighter than the secondary.
Below is a table with star system details from the Washington Double Star (WDS) Catalog. This catalog is a comprehensive source of information on double and multiple star systems, providing key data on the positions, magnitudes, and separations of stellar components.
Technical Details of Star System 10435+4612
| Property | Value |
|---|---|
| Star System Identifier | 10435+4612 |
| System Type | 8-star Star System |
| Primary Star | UMa-10435 4612 |
| Right Ascension (RA) | 10.72578 (10h 43m 32s") |
| Declination (Dec) | 46.20386 (46° 12' 13s) |
| Magnitude (Primary) | 5.21 |
| Magnitude (Secondary) | 7.35 |
| Spectral Type (Primary/Secondary) | F5III |
| Separation (Arcseconds) | 288.1 |
| Position Angle | 88° |
| Discovery Year | 1874 |
| Last Observed | 2018 |
| Primary Proper Motion (Ra, Dec) | -270-066 |
| Secondary Proper Motion (Ra, Dec) | -271-064 |
| Number of Observations | 25 |
10435+4612 Components
| Component | Magnitude | Separation (arcseconds) | Position Angle |
| AB | 7.35 | 288.1 | 88 |
| AC | 11.11 | 139.3 | 5 |
| AD | 9.18 | 375.9 | 43 |
| BD | 9.18 | 273.1 | 350 |
| BE | 10.46 | 2.9 | 291 |
| BF | 14.79 | 11.2 | 152 |
| BP | 13.55 | 120.0 | 270 |
Notes
The data presented in this table is sourced from the Washington Double Star (WDS) Catalog, a comprehensive repository of double and multiple star system information maintained by the U.S. Naval Observatory. We thank the WDS team for their continued efforts in providing accurate and detailed astronomical data.
Finder Chart for
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| Object name | 10435+4612 |
| Field of view | |
| Limiting magnitude | |
| 10435+4612 coordinates | 10.72578, 46.20386 |
| Center coordinates | 10.72578, 46.20386 |
10435+4612 Passage Through Night
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Current position of 10435+4612
| Time | 13:47 |
| Latitude | 39.9625 |
| Longitude | -83.0061 |
| 10435+4612 elevation | 22° |
| 10435+4612 Azimuth | -48° |
Here you can see the current position of the 10435+4612 on the map, as well as its positions for rise and set. This tool allows you to track the 10435+4612's movement throughout the night, providing you with accurate and up-to-date information.
Annual motion of 10435+4612
| Date | Tue, 20 May 2025 |
| Twighlight start | 22:33 |
| Twighlight end | 04:14 |
| Twighlight duration | 6h 41m |
| Rise | 10:17 |
| Set | 06:21 |
| Elevation at transit | 84° |
| Transit time | 20:19 |
| Equatorial coordinates | RA: 10h 43m 32s", Dec: 46° 12' 13s |
| Magnitude | 5 |
| Constellation | Ursa Major |
The graph illustrates the annual visibility pattern of a 10435+4612, 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 10435+4612 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 10435+4612 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.