Double Star 13470+3833 Observation Details
13470+3833 Daily Motion
13470+3833 will be visible until September, 24, 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.
13470+3833 Visibility Timetable on May 09
13470+3833 Rise and Set Timetable
| Time | Elevation | |
| 13470+3833 rise | 15:38 | |
| Moon Rise, 87.7% illuminated | 17:00 | 11° |
| Sunset | 20:27 | 47° |
| Civil sunset | 20:57 | 53° |
| Astrosession begin | 22:10 | 67° |
| 13470+3833 transit | 00:09 | 89° |
| Astrosession end | 04:44 | 37° |
| Moon Set | 04:47 | 37° |
| Civil sunrise | 05:57 | 24° |
| Sunrise | 06:28 | 19° |
| 13470+3833 set | 08:40 |
Track 13470+3833 Position Throughout the Night
← Fri, 9 May 2025 →
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Shift the map to change the time and observe 13470+3833 changing position in the night sky.
13470+3833 Star System Description
13470+3833 is Triple Star System located in constellation Canes Venatici at coordinates RA: 13h 46m 59s", Dec: 38° 32' 33s.
The primary component has a magnitude of 5.62, while the secondary component has a magnitude of 8.91. They are separated by 1.2 arcminute at a position angle of 238 degrees. The brightness difference between the two components is 3.29 magnitudes, with the primary component being approximately 20.7 times brighter than the secondary.
The primary star is orange in color, and the secondary star is yellow-white.
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.
V: Proper motion or other technique indicates that this pair is physical.
The primary component has a magnitude of 5.62, while the secondary component has a magnitude of 8.91. They are separated by 1.2 arcminute at a position angle of 238 degrees. The brightness difference between the two components is 3.29 magnitudes, with the primary component being approximately 20.7 times brighter than the secondary.
The primary star is orange in color, and the secondary star is yellow-white.
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 13470+3833
| Property | Value |
|---|---|
| Star System Identifier | 13470+3833 |
| System Type | Triple Star System |
| Primary Star | CVn-13470 3833 |
| Right Ascension (RA) | 13.78325 (13h 46m 59s") |
| Declination (Dec) | 38.54269 (38° 32' 33s) |
| Magnitude (Primary) | 5.62 |
| Magnitude (Secondary) | 8.91 |
| Spectral Type (Primary/Secondary) | K0III+F8V (orange/yellow-white) |
| Separation (Arcseconds) | 71.3 |
| Position Angle | 238° |
| Discovery Year | 1825 |
| Last Observed | 2018 |
| Primary Proper Motion (Ra, Dec) | -134-021 |
| Secondary Proper Motion (Ra, Dec) | -137-022 |
| Number of Observations | 36 |
13470+3833 Components
| Component | Magnitude | Separation (arcseconds) | Position Angle |
| AB | 8.91 | 71.3 | 238 |
| AC | 8.93 | 999.9 | 296 |
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 | 13470+3833 |
| Field of view | |
| Limiting magnitude | |
| 13470+3833 coordinates | 13.78325, 38.54269 |
| Center coordinates | 13.78325, 38.54269 |
13470+3833 Passage Through Night
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Current position of 13470+3833
| Time | 03:43 |
| Latitude | 37.751 |
| Longitude | -97.822 |
| 13470+3833 elevation | 48° |
| 13470+3833 Azimuth | 72° |
Here you can see the current position of the 13470+3833 on the map, as well as its positions for rise and set. This tool allows you to track the 13470+3833's movement throughout the night, providing you with accurate and up-to-date information.
Annual motion of 13470+3833
| Date | Sat, 10 May 2025 |
| Twighlight start | 22:07 |
| Twighlight end | 04:38 |
| Twighlight duration | 7h 31m |
| Rise | 15:34 |
| Set | 08:36 |
| Elevation at transit | 89° |
| Transit time | 00:05 |
| Equatorial coordinates | RA: 13h 46m 59s", Dec: 38° 32' 33s |
| Magnitude | 6 |
| Constellation | Canes Venatici |
The graph illustrates the annual visibility pattern of a 13470+3833, 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 13470+3833 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 13470+3833 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.