How do you measure the parallax of a star?
You compare two measurements of the position of a star as seem against the general background.
In order to measure parallax, you need two points that are known to be apart in distance.
The result is more accurate the larger the base (distance).
The largest possible base comes from two opposing points on Earth's orbit; in that case, the base is roughly 300 million kilometers across.
Note: To see how your finger moves in relation to the background, place it at arm's length and look with one eye first, then the other. You will notice that your base is approximately 7 cm!
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When a star is observed to have changed apparent position as the Earth orbits the Sun, this shift is known as parallax and can be used to calculate the star's distance using simple geometry and the known distance between the Earth and the Sun. The shift is measured by taking pictures of the star at different times of the year when the Earth is on opposite sides of its orbit and calculating the angle of shift using trigonometry.
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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.
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