Are Wet, Rocky Planets Common in the Universe?

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SUMMARY

Wet, rocky planets are suggested to be common in the universe based on indirect evidence, as discussed in Lineweaver's article from September 2002. The term M*sin(i) refers to the mass of an exoplanet, where 'i' represents the orbital inclination relative to the observer. This inclination affects the observed wobble of the star due to the Doppler effect, leading to systematic underestimation of the planet's mass. Accurate mass determination occurs only in specific cases where the planet transits in front of the star, allowing for precise measurement of both mass and inclination.

PREREQUISITES
  • Understanding of exoplanet detection methods, particularly Doppler spectroscopy
  • Familiarity with orbital mechanics and inclination concepts
  • Knowledge of light curves and their significance in astronomy
  • Basic grasp of mass estimation techniques in astrophysics
NEXT STEPS
  • Research the principles of Doppler spectroscopy in exoplanet detection
  • Study the mathematical implications of orbital inclination on mass estimation
  • Explore case studies of transiting exoplanets and their light curves
  • Investigate the significance of M*sin(i) in current astrophysical models
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Astronomers, astrophysics students, and anyone interested in exoplanet research and the methods used to determine planetary masses.

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http://arxiv.org/abs/astro-ph/0209383

"Much indirect evidence suggests that wet, rocky planets are common."

fairly recent article by Lineweaver (September 2002)
 
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Hmm, interesting. Just two questions for now. What does he mean by the i in M*sin(i)? And what's the significance of M*sin(i). Afraid I've not come across this before.
 
Originally posted by Lonewolf
Hmm, interesting. Just two questions for now. What does he mean by the i in M*sin(i)? And what's the significance of M*sin(i). Afraid I've not come across this before.

this is a standard term in the exoplanet search (exosolar planet search) where i is the inclination of the orbit relative to the observer

in most cases the planet is detected by wobble, changes in the radial speed of the star, by doppler effect

If the observer is in the plane of the star and planet two-body motion (inclination = 0) then one measures the whole wobble

if the inclination is 90 degrees one wouild not see any wobble

in general the inclination is unknown and one sees a fraction of the wobble which is sine(inclination).

therefore one systematically underestimates the mass of the planet, in fact ones estimate of the mass is only sin(i) times the mass, where the inclination is an unknown number between zero and one

and so the tables show sin(i)M because one cannot actually say anything about M itself

as parttime astronomer you will see that the mass of the star itself is told by the color etc. -----so knowing the period will tell the distance from the star and knowing the wobblespeed and the distance will tell the mass of the planet----but one only knows sine(inclination) X wobblespeed

EXCEPT in a few cases where the planet actually passes in front of the disk of the star and notches the lightcurve----there are a few of these inclination=0 cases where one has two handles on the problem
 

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