Light from the sun reaches Earth in 8.3 min. The velocity of light is 3.00 108 m/s. Given this info, how would you determine how far the Earth is from the sun?

Answer 1

#d = 1.49 xx 10^11 "m"#

The distance formula can be used to find velocity, which is defined as the rate of travel.

#"velocity" = "distance"/"time"#

By rearranging this formula, we can find the distance given the travel time and velocity.

#d = vt#

Since we know the velocity and time, we can solve for the distance, but if we enter the provided values;

#d= (3.00 xx 10^8 "m/s")(8.3"minutes")#

Since seconds are the SI unit for time, we must convert 8.3 minutes to seconds as we can see that the units are out of alignment.

#t = (8.3 "minutes")(60 "seconds/minute")=(498 "s")#

We can now solve for distance because our units match up.

#d = (3.00 xx 10^8 "m/s")(498 "s")#
#d = 1.49 xx 10^11 "m"#
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Answer 2

You can use the following formula to find the distance between the Earth and the Sun: Distance = Velocity of light × Time taken for light to travel. Substitute the given values to get the following result: Distance = (3.00 × 10^8 m/s) × (8.3 min × 60 s/min) ≈ 2.5 × 10^11 meters. This indicates that the Earth is roughly 2.5 × 10^11 meters from the Sun.

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Answer from HIX Tutor

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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