Help with Astronomy 101 Questions: Orbit Radius & Angular Diameter

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SUMMARY

This discussion addresses two fundamental questions in Astronomy 101 regarding circular velocity and angular diameter. The circular velocity of a satellite orbiting Earth at a radius of 4,000,000 meters is calculated using the formula v = √(GM/r), resulting in approximately 7,673 m/s. Additionally, the angular diameter of an object with a linear diameter of 2,250 km at a distance of 4,000,000 km is determined using θ = 2arctan(d/2D), yielding an angular diameter of approximately 0.032 degrees.

PREREQUISITES
  • Understanding of gravitational constant (G = 6.67 x 10^-11 Nm^2/kg^2)
  • Familiarity with the mass of Earth (M = 5.97 x 10^24 kg)
  • Knowledge of trigonometric functions, specifically arctan
  • Basic concepts of orbital mechanics
NEXT STEPS
  • Study the derivation of the circular velocity formula in orbital mechanics
  • Learn about the implications of angular diameter in astronomy
  • Explore the concept of gravitational forces and their effects on satellite motion
  • Investigate the applications of trigonometry in astronomical measurements
USEFUL FOR

Astronomy students, educators, and anyone interested in understanding the principles of orbital mechanics and angular measurements in space.

msyvette
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I need help please. i have a couple of questions if someone could please help me with.

1. If a satellite with a small mass (any #) is orbiting the Earth with an orbit radius of 4000000m, what is the circular velocity of the satellite?

2. if the distance to an object is 4000000 km and the linear diameter if the same object is 2250 km, what is the angular diameter of the object in degrees?
 
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What formulas do you think might apply here? Have you drawn a picture for the second one?

Sorry I can't be more helpful... forum rules that we won't do homework for you.

Post what you've tried - we'll be more than happy to help you a bit more.
 


Sure, I'd be happy to help with your questions about orbit radius and angular diameter in Astronomy 101. Here are the answers to your two questions:

1. The circular velocity of a satellite in orbit is determined by the formula v = √(GM/r), where G is the gravitational constant (6.67 x 10^-11 Nm^2/kg^2), M is the mass of the central body (in this case, the Earth), and r is the orbit radius. Plugging in the values given, we get v = √((6.67 x 10^-11 Nm^2/kg^2)(5.97 x 10^24 kg)/4000000m) = 7673 m/s. So the circular velocity of the satellite is approximately 7673 m/s.

2. The angular diameter of an object can be calculated using the formula θ = 2arctan(d/2D), where d is the linear diameter of the object and D is the distance to the object. Plugging in the values given, we get θ = 2arctan((2250 km/2)/(4000000 km)) = 0.032 degrees. So the angular diameter of the object is approximately 0.032 degrees.

I hope this helps! If you have any further questions, please feel free to ask. Good luck with your studies in Astronomy 101!
 

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