How Do You Solve These Astronomy Homework Problems?

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SUMMARY

This discussion focuses on solving specific astronomy homework problems involving parallax, luminosity, and orbital velocity. The first problem requires calculating the distance and absolute magnitude of a star with a parallax of 0.016 arc seconds and an apparent magnitude of 6. The second problem involves determining the luminosity of a star that is 10 times the radius of the Sun and half as hot. The final problem addresses the diameter of an eclipsing binary star with an orbital velocity of 153 km/s and an eclipse duration of 2.5 hours.

PREREQUISITES
  • Understanding of parallax and its relation to distance in astronomy
  • Knowledge of absolute magnitude calculations
  • Familiarity with the Stefan-Boltzmann Law for luminosity
  • Basic concepts of binary star systems and orbital mechanics
NEXT STEPS
  • Study the parallax formula and its application in distance measurement
  • Learn about the Stefan-Boltzmann Law to calculate stellar luminosity
  • Research methods for determining the diameter of stars in binary systems
  • Explore the concept of apparent vs. absolute magnitude in detail
USEFUL FOR

Astronomy students, educators, and anyone interested in solving problems related to stellar measurements and properties.

PhysicsMajor86
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I cannot figure out the answers for the following problems:

1) If a star has a parrallax of 0.016 second of arc and an apparent magnitude of 6, how far away is it, and what is its absolute magnitude?

7) If a star is 10 times the radius of the sun and half as hot, what will its luminosity be?

13) If the orbital velocity of the eclipsing binary in Figure 8-17 is 153 km/s and the smaller star becomes completely eclipsed in 2.5 hours, what is its diameter?
 
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