Proving Venus's Orbit is 0.72x Earth's: Understanding Greatest Elongation

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SUMMARY

Venus's orbit is confirmed to be 0.72 times the size of Earth's orbit, based on its greatest elongation of 47 degrees. The mean distance from the Sun to Venus is 108,200,000 km (0.72 AU), with an eccentricity of 0.007 and an inclination of 3.4° to the ecliptic. The calculation of 0.73 AU using trigonometric functions aligns closely with the mean distance, highlighting the distinction between mean and maximum distances in orbital mechanics.

PREREQUISITES
  • Understanding of trigonometric functions, specifically sine.
  • Familiarity with astronomical units (AU) and their application in planetary distances.
  • Knowledge of orbital mechanics, including concepts like eccentricity and inclination.
  • Basic understanding of planetary data and characteristics, such as mass and density.
NEXT STEPS
  • Research the calculation of orbital distances using trigonometry in celestial mechanics.
  • Explore the significance of eccentricity in planetary orbits, particularly for Venus.
  • Study the concept of greatest elongation and its implications for observational astronomy.
  • Learn about the differences between mean and maximum distances in planetary orbits.
USEFUL FOR

Astronomers, astrophysics students, and anyone interested in planetary science and orbital dynamics will benefit from this discussion.

ahirschey
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Prove that Venus’s orbit is .72 times the size of Earth's orbit. I’m told that Venus’s greatest elongation is 47 degrees.
 
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Planetary data for Venus
mean distance from Sun 108,200,000 km (0.72 AU)
eccentricity of orbit 0.007
inclination of orbit to ecliptic 3.4°
Venusian year (sidereal period of revolution) 224.7 Earth days
maximum visual magnitude –4.6
mean synodic period* 584 Earth days
mean orbital velocity 35 km/s
radius (equatorial and polar) 6,051.8 km
surface area 4.6 × 108 km2
mass 4.87 × 1024 kg
mean density 5.25 g/cm3
mean surface gravity 860 cm/s2
escape velocity 10.4 km/s
rotation period (Venusian sidereal day) 243 Earth days (retrograde)
Venusian mean solar day 116.8 Earth days
inclination of equator to orbit 177°
atmospheric composition carbon dioxide, 96%; molecular nitrogen, 3.5%; water, 0.02%; trace quantities of carbon monoxide, molecular oxygen, sulfur dioxide, hydrogen chloride, and other gases
mean surface temperature 737 K (867 °F, 464 °C)
surface pressure at mean radius 95 bars
mean visible cloud temperature about 230 K (–46 °F, –43 °C)
number of known moons none

*Time required for the planet to return to the same position in the sky relative to the Sun as seen from Earth.
 
Venus is at greatest elongation when the sun - venus - Earth system makes a 90 degree angle at venus's position. Knowing the distance from the Earth to the sun is 1AU, and using some trig, sin(47)*1AU ~ 0.73AU. The reason that this is .01 off of given, is because that given value is the mean distance, not the maximum distance which is what was calculated using the given information.
 

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