Local Sidereal Time, RA of a star

In summary, a star on the celestial equator with a right ascension of 16h00m00s will be at its highest point on February 29th, 2016 at approximately 4:00 am. This can be determined by calculating the Local Sidereal Time (LST) using the formula HA = LST - RA, and taking into account a rough estimate of a 4 minute difference between solar and sidereal time. This estimate may vary based on the date and time of observation.
  • #1
bunchedupwalrus
9
0

Homework Statement


*A star on the celestial equator has right ascension of 16h00m00s. At what time of day will this star be at it's highest point, on Febuary 29th 2016. *

Homework Equations


HA = LST - RA

The Attempt at a Solution



When LST=RA, it'll be at it's highest point. How do I determine LST? There are many different explanations online. As a rough estimate, solar is off from sidereal by 4 minutes. 0 hour is on March 20th. Subtracting 4 minutes per day for 20 days gives me a difference of about 80 minutes.

So it'd be 16h - (80minutes), roughly 2pm?
 
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  • #2
bunchedupwalrus said:
When LST=RA, it'll be at it's highest point.
Correct.
As a rough estimate, solar is off from sidereal by 4 minutes.
Correct.
0 hour is on March 20th.
Not correct. The sun is at 0h RA at the Vernal Equinox, roughly March 20. So when the sun is at its highest point on Mar 20, this is 0h LST. But the sun is at its highest point at 12h solar time, not 0h solar time. So there is an additional 12h offset.
 
  • #3
I'd try drawing a sketch of the situation.

Also, consider this: on March 20, the star will be highest in the sky at 4 am. A day earlier, it would have risen 4 minutes later, so it would be highest around 4:04 am, right? Your answer of 2 pm can't be right, even ignoring the am/pm difference.
 

Related to Local Sidereal Time, RA of a star

1. What is Local Sidereal Time (LST)?

Local Sidereal Time (LST) is a measurement of the Earth's rotation with respect to the stars. It is based on the position of the vernal equinox (the point at which the celestial equator intersects with the ecliptic) and is used as a reference for determining the Right Ascension (RA) of a star.

2. How is LST calculated?

LST is calculated by taking into account the Earth's rotation period of approximately 23 hours and 56 minutes, as well as the Earth's precession and nutation. It can be calculated using a formula that takes into account the observer's longitude, the time since the vernal equinox, and the Earth's rotation rate.

3. What is the significance of LST in astronomy?

LST is significant in astronomy because it allows astronomers to determine the position of a celestial object in the sky at a specific time and location. This is important for making accurate observations and for coordinating observations between different observatories.

4. How does LST differ from Local Time?

LST and Local Time differ because LST is based on the Earth's rotation with respect to the stars, while Local Time is based on the Earth's rotation with respect to the Sun. This means that LST is a constant reference point, while Local Time can vary depending on the observer's location on Earth.

5. How is LST used to determine the RA of a star?

LST is used to determine the RA of a star by providing a reference for the Earth's rotation and the position of the vernal equinox. By knowing the LST and the current time, an astronomer can calculate the RA of a star using a formula that takes into account the Earth's rotation rate and the time since the vernal equinox.

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