Detecting Jupiter-like Planets Using the Doppler Effect

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SUMMARY

The discussion focuses on detecting Jupiter-like planets using the Doppler effect, emphasizing the precision of radial velocity measurements at 1 m/s. The mass of Jupiter (1.898 x 10^27 kg) and the Sun (1.989 x 10^30 kg), along with the distance between them (778,500,000 km), are critical data points. The equations for radial velocity and the relationship between the semimajor axes of the Sun and the planet are highlighted as essential for calculations. Kepler's laws may also provide useful insights for this analysis.

PREREQUISITES
  • Understanding of the Doppler effect in astrophysics
  • Familiarity with radial velocity measurements
  • Knowledge of Kepler's laws of planetary motion
  • Basic grasp of gravitational physics and mass calculations
NEXT STEPS
  • Research the application of the Doppler effect in exoplanet detection
  • Study the mathematical derivation of radial velocity equations
  • Explore Kepler's laws and their implications for planetary orbits
  • Investigate current technologies used for measuring radial velocities in astronomy
USEFUL FOR

Astronomers, astrophysics students, and researchers interested in exoplanet detection and the application of the Doppler effect in measuring celestial bodies' movements.

adgar
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Homework Statement

The precision in measurements of radial velocities by the Doppler effect is currently 1 m/s.
Can a Jupiter like planet orbiting a star similar to the Sun at a distance from the mother star equal to the Sun-Jupiter distance be detected?'
(Use www or other sources to find the mass of Jupiter, the Sun and the distance between the two which are the only data you are allowed to use).

Ms = 1.989*10^30 kg
Mj = 1.898*10^27 kg
d = 778500000 km

Homework Equations


|vr|= v sin(i), where
vr is the radial velocity
v is the real velocity
and i is the inclination of the orbit.

a*/ap = v*/vp = v*r/vpr
where a* and ap are the semimajor axis of the sun and the planet.

Kepler's 3. low can maybe be usefull.

The Attempt at a Solution

 
Last edited:
Physics news on Phys.org
Hello ad and welcome to PF.
Did you notice PF requires the use of the template (which somehow you circumvaded) ? Ýou got as far as point 1. Now 2 and 3, please !
 

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