18. What is meant by an exoplanet being in a “resonant orbit”?
- A) Its orbit matches the rotation rate of its host star
- B) Its orbit is in a simple integer ratio with another planet’s orbit
- C) It has an eccentric orbit that changes due to tidal forces
- D) It oscillates in brightness due to its atmospheric composition
Answer: D) It oscillates in brightness due to its atmospheric composition
Some exoplanets’ brightness changes periodically due to cloud patterns, heat distribution, or atmospheric chemistry.
20. What is an active galactic nucleus (AGN)?
- A) The core of a galaxy containing a supermassive black hole that emits large amounts of energy
- B) A dense cluster of neutron stars at the center of a galaxy
- C) The rotating disk of young stars in the galactic core
- D) The remnant of a galaxy that has merged with another
Answer: A) The core of a galaxy containing a supermassive black hole that emits large amounts of energy
An AGN’s extreme luminosity comes from matter accreting onto the black hole, producing radiation across the electromagnetic spectrum.
Bonus: What makes NASA’s Pandora mission uniquely suited to disentangling stellar variability from exoplanet transit signals?
- A) It uses a coronagraph to block out starlight for direct imaging
- B) It observes exoplanet systems from two different planets simultaneously
- C) It observes an exoplanet system continuously for at least 24 hours, repeating the process 10 times
- D) It only targets stars without sunspots or variability
Answer: C) It observes an exoplanet system continuously for at least 24 hours, repeating the process 10 times
Pandora simultaneously measures the star’s light in visible and infrared wavelengths for an entire 24-hour span, returning to observe the same system multiple times. This long-duration, repeated approach allows scientists to characterize how the star’s own variability (spots, flares, faculae) affects the measured transit depth, improving the accuracy of exoplanet atmosphere studies.