A star is observed to have the following equatorial coordinates:
- Right Ascension (RA): 5 hours 34 minutes 12 seconds
- Declination (Dec): 22 deg 15 arcmin 48 arcsec
- Convert the Right Ascension (RA) from hours, minutes, and seconds into decimal degrees.
- Determine the star's position in the sky relative to the Celestial Equator (is it north or south of the equator?).
- If the Local Sidereal Time (LST) at your location is 3 hours 45 minutes, calculate the hour angle of the star.
1. Convert RA to decimal degrees:
- RA = 5 hours 34 minutes 12 seconds
- Convert hours, minutes, and seconds to decimal degrees:
hour |
since hours |
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minute |
since minutes |
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second |
since seconds |
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- RA in decimal degrees:
hours |
 |
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minutes |
 |
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seconds |
 |
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Total RA |
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2. Determine the star's position relative to the celestial equator:
- Declination (Dec) = 22 deg 15 arcmin 48 arcsec
- Since the declination is positive, the star is north of the celestial equator.
3. Calculate the hour angle (HA):
- Local Sidereal Time (LST) = 3 hours 45 minutes
- Convert LST to decimal degrees:
- Hour Angle (HA) = LST - RA
HA |
 |
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- A negative hour angle means the star is east of the meridian (not yet crossed the observer's meridian).
This example was generated by DeepSeek, an AI, on February 25, 2025.
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