What makes stellar parallax easier to observe?
Because when readings are taken at two different times, simple geometry allows for the calculation
The stellar parallax is good but is limited. For astronomers to make their calculation the measured angle can be no less than 1 arc second.
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Larger baselines make observing stellar parallax easier. For example, if two points are farther apart, the star can be observed from both ends of Earth's orbit around the Sun, which yields a baseline of about two astronomical units (AU). Accurate measurements of stellar parallax have also been made possible by advances in telescopic technology and precision instruments.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
- Which type of galaxy has stars that are symmetrically dispersed in a spherical or flattened shape?
- If over billions of years of time and many collisions with other galaxies, would the collection of supermassive black hole be enough to destroy all the mass of the billion of years of collected stars?
- Why is stellar parallax important?
- What is the parallax angle?
- What causes a massive star to explode?
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