A star has a parallax of .05. What is its distance?
distance = 1/p where p is parallax angle in arc sec and d in parsec.
The distance is 2 parsecs, or 6.52 light years, according to 1/p=1/0.5=2.
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To find the distance to the star, use the formula: distance (in parsecs) = 1 / parallax angle (in arcseconds). So, distance = 1 / 0.05 = 20 parsecs.
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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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