Most of the extrasolar planets found so far were detected by
A) noting the drop in the star’s light as the planet transits its disk.
B) imaging them with the HST in the infrared, where they are easier to stop.
C) noting the Doppler shifts of the star as the planet orbits it from side to side.
D) receiving radio transmissions from them, much like Jupiter emits.
E) detecting the oxygen in their atmospheres spectroscopically.
The Oort Cloud is believed to be
A) a flattened belt of cometary nuclei just beyond the orbit of Neptune.
B) the circular disk of gas around the Sun’s equator from which the planets formed.
C) a grouping of asteroids and meteoroids between the orbits of Mars and Jupiter.
D) a spherical cloud of cometary nuclei far beyond the Kuiper Belt.
E) the great nebula found just below the belt stars of Orion.