Solar Systems Flashcards
Give some differences between terrestrial and jovian planets.
Terrestrial: Less than 2AU from Sun
Small
Mostly rocky materials
High Density
Jovian: More than 5AU from Sun
Large
Mostly light H and He
Low Density
T or F. Mercury has no atmosphere.
True.
What is the primary element in the atmosphere of Venus and Mars?
Carbon Dioxide.
Formula for kinetic energy of a gas atom or molecule.
E = ( 3 / 2 )* (B) * T
E = energy
T = temperature
B = Boltzmann Constant
Formula for average speed of a gas atom or molecule.
root( 3 * (B) * T / m)
where T = Temperature
m = mass
B = Boltzmann Constant
T or F. All the jovian planets have rings.
True.
How are planetary rings formed?
When a satellite passes inside the roche limit, the tidal forces overwhelm the gravitational forces that hold the satellite together. The fragments are spread about the planet by Kepler’s third law.
How is the Roche limit of a planet calculated?
2.4 * radius
Name two features of Jupiter.
Aurorae on its poles
Great red spot
T or F. Jupiter’s atmosphere does not seem to suffer significant changes over the years.
False.
T or F. The smallest size of the Great Red Spot is one earth diameter.
True.
What is unique about Uranus?
Its axis of rotation is fully tilted with the equatorial plane perpendicular to the orbital plane.
T or F. Despite its rotation being tilted, all of Uranus’ satellites still orbit around Uranus along the orbital plane.
False.
Why are features not easily seen on the surface of Uranus?
Features form in the troposphere closer to the surface.
T or F. If you wanted to see planets in Dublin’s night sky you should look at the ecliptic?
True.
T or F. From the terrestial planets, only Venus and Earth have atmospheres.
False.
T or F. Venus has no magnetic field.
True.
T or F. Mars and Mercury have magnetic fields though weak.
True.
T or F. The magnetic field of Earth is of moderate strength like Mars.
False.
Name four methods for detecting exoplanets.
Radial velocity or ‘stellar wobble’ method.
Astrometric method
Transit Photometry
Direct Imaging
Explain how radial velocity method works.
If a star has companions, then the wavelengths of the stars spectral lines get Doppler shifted, since the star has motion relative to the centre of mass of the solar system.
The magnitude of the wobble determines the companion minimum mass, the period determines the semimajor axis.