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Orbital Dynamics of Venus (and some of those other things out there) Billy Teets, PhD Candidate Dept. of Physics & Astronomy Vanderbilt University.

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Presentation on theme: "Orbital Dynamics of Venus (and some of those other things out there) Billy Teets, PhD Candidate Dept. of Physics & Astronomy Vanderbilt University."— Presentation transcript:

1 Orbital Dynamics of Venus (and some of those other things out there) Billy Teets, PhD Candidate Dept. of Physics & Astronomy Vanderbilt University

2 Orbital Period – 225 Days Sidereal Day – 243 Days Eccentricity – 0.0068 Tilt – 177° Oblateness ~ 0.00 Surface Pressure – 90 bars Average Temperature – 850 °F – 470 °C Atmospheric Composition – 97% CO 2 Orbital Dynamics Planet Characteristics Venus

3 Phases of Venus

4 Determining the Distance to Venus Using Phase

5 Transits of Venus

6 Transit Timings 122 years 8 years 105 years 8 years Orbital Resonances (Venus:Earth) 395:243 13:8 Transits of Venus

7 Other Orbital Resonances: Jupiter’s Moons

8 Other Orbital Resonances: Saturn’s Moons and Rings

9 Mimas& Saturn

10 Other Orbital Resonances: Organization of the Early Solar System

11 Retrograde Motion: Jupiter & Saturn

12 Retrograde Motion: Mars

13 Retrograde Motion: Epicycle &Deferent

14 Retrograde Motion: Heliocentric View

15

16 Lagrange Points and Trojan Asteroids

17 Lagrange Points: STEREO A&B Probes


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