Comparing Angular Rates of Star Rotation at Different Latitudes and Longitudes

Additionally, taking into account precession and the viewer's position on Earth, the stars at the poles move much slower in apparent velocity than those at the equator.
  • #1
Philosophaie
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The Earth's rotational velocity at the Equator is 1,674.4 km/h or 465.1 m/s. The stars at the equator rotate at that same rate taking in account Precession at that particular time of the year and the longitude & latitude they are viewed from. Do the stars at the poles rotate faster then at the equator also depending the longitude & latitude they are viewed from?
 
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  • #2
No. Another way of looking at it by imagining the sky is rotating around the Earth instead. The stars near the poles move much slower in apparent velocity than the ones near the equator do.
 
  • #3
Philosophaie said:
The Earth's rotational velocity at the Equator is 1,674.4 km/h or 465.1 m/s. The stars at the equator rotate at that same rate

No, be careful. It makes no sense to compare the linear rates (the stars don't move at 1674 km/h). It's the angular rate (of about 15 degrees/hr) that is the same.
 

Related to Comparing Angular Rates of Star Rotation at Different Latitudes and Longitudes

1. What is the rotational velocity of stars?

The rotational velocity of stars refers to the speed at which a star rotates on its axis. This can vary greatly depending on the size and mass of the star, with larger and more massive stars generally having a higher rotational velocity.

2. How is the rotational velocity of stars measured?

The rotational velocity of stars is typically measured using spectroscopy. By studying the Doppler shift of spectral lines, scientists can determine the rotational velocity of a star. This technique is most effective for stars that have a high rotational velocity and are close to Earth.

3. What factors affect the rotational velocity of stars?

The rotational velocity of stars can be influenced by a variety of factors, including the star's mass, age, and composition. For example, younger stars tend to have a higher rotational velocity due to their rapid rotation during their formation process.

4. Can the rotational velocity of stars change over time?

Yes, the rotational velocity of stars can change over time. For example, as a star ages, it may slow down its rotation due to the loss of angular momentum through stellar winds. Additionally, interactions with other stars or planets can also affect a star's rotational velocity.

5. How does the rotational velocity of stars affect their lifespan?

The rotational velocity of stars can have a significant impact on their lifespan. Faster rotating stars tend to have shorter lifespans, as the centrifugal force from their high rotational velocity can cause them to lose mass more quickly. This can lead to the star running out of fuel and eventually dying sooner than a slower rotating star.

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