Astronomy homework, right ascension

In summary, the right ascension of a star does not change, but the position of the sun changes throughout the year. Due to this change, the star will set 15 minutes after the sun has set and will not be visible in the night sky at the specified latitude during dark hours.
  • #1
petha1
5
1
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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  • #2
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.
 
  • #3
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.
 

FAQ: Astronomy homework, right ascension

What is right ascension in astronomy?

Right ascension is a celestial coordinate used in astronomy to locate objects in the sky. It is measured in hours, minutes, and seconds and is equivalent to longitude on Earth. It is used in conjunction with declination, which is equivalent to latitude on Earth, to pinpoint the location of objects in the sky.

How is right ascension measured?

Right ascension is measured along the celestial equator, which is an imaginary line that divides the sky into northern and southern hemispheres. It is measured eastward from the vernal equinox, which is the point where the celestial equator intersects with the ecliptic, the apparent path of the Sun in the sky.

What is the unit of measurement for right ascension?

The unit of measurement for right ascension is hours, minutes, and seconds. One hour of right ascension is equivalent to 15 degrees of longitude on Earth, and one minute of right ascension is equivalent to 15 minutes of longitude.

How is right ascension different from declination?

Right ascension and declination are both celestial coordinates used to locate objects in the sky. However, right ascension is measured along the celestial equator, while declination is measured along the celestial meridian. Right ascension is also measured in hours, minutes, and seconds, while declination is measured in degrees, minutes, and seconds.

Why is right ascension important in astronomy?

Right ascension, along with declination, is used to create a coordinate system that allows astronomers to locate objects in the sky. This is important for observing and studying celestial objects, as well as for navigation and timekeeping. Right ascension is also used to determine the rising and setting times of objects in the sky, and to track their movements over time.

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