Time of sunset using Radius of earth

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SUMMARY

The discussion focuses on calculating the time until sunset based on the observer's height above the ground and the Earth's radius. The radius of the Earth is established as 6400 km, and the observer's height changes from 20 cm to 170 cm. The correct approach involves using the arccosine function to determine the angle of the Earth's curvature, leading to a calculation of time using the formula: time = (angle in radians / 2π) * 86400 seconds. The final calculation yields approximately 9.41 seconds for the observer to see the Sun disappear again.

PREREQUISITES
  • Understanding of basic trigonometry, specifically the arccosine function.
  • Familiarity with the geometry of circles and angles.
  • Knowledge of the Earth's radius (6400 km) and its implications for horizon calculations.
  • Basic principles of celestial motion and the Sun's path across the sky.
NEXT STEPS
  • Study the application of the arccosine function in real-world scenarios.
  • Learn about the geometry of circles and how it relates to horizon visibility.
  • Research the effects of observer height on sunset calculations.
  • Explore the concept of solar motion and its impact on sunset timing.
USEFUL FOR

Students in physics or mathematics, educators teaching trigonometry and geometry, and anyone interested in understanding the relationship between observer height and sunset timing.

George3
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URGENT Time of sunset using Radius of earth

Homework Statement



The Sun sets, fully disappearing over the horizon as you lie on the beach, your eyes 20 cm above the sand. You immediately jump up, your eyes now 170 cm above the sand, and you can again see the top of the Sun. If you count the number of seconds ( = t) until the Sun fully disappears again, you can estimate the radius of the Earth. Use the known radius of the Earth to calculate the time t.

2 sig figs

Homework Equations





The Attempt at a Solution


radius = 6400m
radius + height = 6400.015
cos(R/(R + h)) = .54 radians
(time/ 1 day) = radians/ 2pi
time = ? I don't think I am doing this right because I am getting like 73000 seconds with this method.
 
Last edited:
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Hi George3! :smile:
George3 said:
radius = 6400m

Small world! :wink:
 
I meant km
 
What is 6400 km + 150 cm?

Edit
Why are you taking the cosine of R/(r+h)?
 
Last edited:
I was taking the cosine of(R/R+h) to find the angle that the Earth moved. Do you have any idea how to tackle this problem?
 
Drawing a picture is often a good start.

Since you are taking the cosine of R/(R+h), it must represent some angle. What is it? (Hint: There is no such angle.)
 
I drew a picture, the line of sight when you are lying down is tangent to the Earth's surface. This would make a right angle with the radius of the earth. Where am I going wrong?
 
R/(R+h) is the ratio of two sides of your triangle. It is not an angle. So why are you taking the cosine of this ratio? You are on the right track but you are using the wrong function.
 
For this problem I did this:
arccos(6400000m/6400001.5m) = .00021radians
.00068radians = .039degrees
.039degrees / 360degrees * 86400secs = 9.41secs
Is this right?
 
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  • #10
Much better.
 
  • #11
This is an online assignment and I only have one more chance to get it right. Should I turn this in or keep working?
 
  • #12
George3 said:
This is an online assignment and I only have one more chance to get it right. Should I turn this in or keep working?

Wait. I don't know how strict your assignment's requirements are, because I haven't seen it, but there's one thing you haven't considered.

You've been assuming that the Sun moves across the sky at 360 degrees per 24 hours, which is (at least approximately) correct, but does it lose altitude at that rate? Think about the Sun's motion: it rises near the east but not exactly due east, arcs its way towards the north or south and reaches due north/south at solar noon, and sets in the west. It doesn't rise in the east and plop right down in the west, so there's a horizontal component of its motion.

You've calculated the minimum possible value of "t". At the poles, where the Sun doesn't set for six months, "t" is on the order of hours or days. If the Earth didn't revolve around the Sun, "t" would be infinite.
 
  • #13
I highly doubt we need to take into consideration of the differences in altitude (just as we prob. don't have to account for the fact that atmosphere bends the light, etc). My attempt at this problem is similar, but with law of sine. And honestly, I can't get this problem either (also at one attempt left).

Lol.

I'll see.
 

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