Calculating Star Visibility: RA and DEC at 09:30 on May 21st

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    Astronomy
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SUMMARY

At 09:30 on May 21st, the Right Ascension (RA) of stars at the zenith can be calculated by considering the local time and the position of the sun. The discussion clarifies that to determine the visibility of a star with an RA of 5 hours, one must add 14.5 hours to the RA at 09:30. The sun's RA remains relatively constant at this time of year, necessitating the use of Universal Time (UT) for accurate calculations. The importance of specifying the observer's location is also emphasized for precise star visibility assessments.

PREREQUISITES
  • Understanding of Right Ascension (RA) and Declination (DEC)
  • Familiarity with celestial navigation concepts
  • Knowledge of time scales such as Universal Time (UT) and Local Time
  • Basic astronomy skills for star visibility calculations
NEXT STEPS
  • Research celestial coordinate systems and their applications in astronomy
  • Learn about the relationship between RA, DEC, and time zones
  • Study the effects of Earth's rotation on star visibility
  • Explore software tools for astronomical calculations, such as Stellarium or SkySafari
USEFUL FOR

Astronomy students, amateur astronomers, and anyone interested in calculating star visibility based on time and location.

Chronos000
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Homework Statement



If at 09:30 21st may what would the RA of stars be at the zenith?

I'm not sure if we can say that they are at 3.5hrs since we are in may?

If a star is at RA 5hrs would at 09:30 would it be observable at 00:00.

My thoughts are that you just add on 14.5 hrs to the RA at 09:30, and we want it to be 12 hours from where the sun would be. but the sun would be at pretty much the same RA
 
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09:30 21st May using what time scale? Local time? (If so, what's your location?) Universal Time? GMT? Dynamical Time?
 

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