Astronomy homework, right ascension

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SUMMARY

The discussion focuses on the calculation of right ascension (RA) in relation to the position of a star and the sun over time. It establishes that the star is 15 minutes and 39.3 seconds behind the sun, indicating it will set shortly after the sun. The right ascension does not change; rather, it is the sun's position that varies throughout the year. The Local Sidereal Time (LST) at midnight is calculated to be 6 hours, which determines the visible right ascensions to be between 04h and 08h.

PREREQUISITES
  • Understanding of right ascension and its significance in astronomy
  • Knowledge of Local Sidereal Time (LST) calculations
  • Familiarity with the concept of the vernal equinox
  • Basic grasp of celestial mechanics and star positioning
NEXT STEPS
  • Research the calculation of Local Sidereal Time (LST) in detail
  • Learn about the effects of the vernal equinox on celestial observations
  • Study the relationship between right ascension and declination
  • Explore tools for tracking celestial objects, such as planetarium software
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Astronomy students, amateur astronomers, and educators looking to deepen their understanding of celestial navigation and star positioning.

petha1
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Homework Statement
Will a star with right ascension of 14h,15m,39,3s be visible on October 21 from a latitude of 56 degrees 53 minutes, 0 seconds? Assume that night is between [22.00,02.00]
Relevant Equations
Right ascension measures how many hours ahead or behind the sun a star is at the vernal equinox, decreses by 2 hours/month.
March 21 - October 21 = 7 months. So the star is only 15m 39,3 seconds behind the sun. This means that the star won't be up when the sun is down.

Answer: No, the star will set only 15 minutes after the sun has set. Therefore it won't be on the sky at the specified latitude during dark hours.

Is this correct reasoning?
 
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petha1 said:
Relevant Equations:: Right ascension measures how many hours ahead or behind the sun a star is at the vernal equinox, decreses by 2 hours/month.
Your answer is correct, but this statement is misleading. The right ascension of a star does not change. It is the position of the sun which changes through the year.
 
Thanks for the help. I think I figured out the correct way to answer this question.
October 21 is 9 months since the vernal equinox. That means that the LST at noon is 18, leading to
the LST at midnight beeing 18+12 = 30 = 6 (mod 24) so the visible RAs are in the range [6-2,6+2] = [4,8]so the visible right ascensions are between 04h and 08h.
 

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