General
Radial Velocity
Transits
Missions
Life in the Universe
100

This method of exoplanet detection involves observing the dimming of a star as a planet passes in front of it.

What is the transit method?

100

This type of light shift is observed when a star moves toward or away from us due to an orbiting planet.

What is the Doppler shift?

100

A planet must have this kind of orbital alignment with respect to Earth for a transit to be observable.

What is edge-on (or nearly edge-on)?

100

The Kepler Space Telescope used this technique to find over 2,600 confirmed exoplanets during its mission.

What is the transit method?

100

This planetary neighbor of Earth has been a primary target in the search for past or present microbial life.

What is Mars?

200

This exoplanet, discovered in 1995, was the first confirmed around a Sun-like star

What is 51 Pegasi b?

200

This part of the star’s spectrum is analyzed for shifts when using the radial velocity technique.

What are absorption lines?

200

The depth of a transit tells us this property of the exoplanet relative to its host star.

What is the planet’s radius (or size)?

200

Kepler focused on a specific region of the sky in this constellation during its primary mission.

What is Cygnus?

200

This icy moon of Jupiter is thought to have a subsurface ocean and is a top candidate in the search for extraterrestrial life.

What is Europa?

300

This region around a star is where liquid water could exist on a planet's surface.

What is the habitable zone?

300

The radial velocity method is most sensitive to planets with these two orbital characteristics.

What are high mass and short orbital period?

300

By measuring the time between transits, scientists can determine this characteristic of an exoplanet's orbit.

What is the orbital period?

300

Launched in 2018, this NASA mission continues the search for exoplanets around bright, nearby stars.

What is TESS (Transiting Exoplanet Survey Satellite)?

300

This famous equation estimates the number of communicative civilizations in our galaxy.

What is the Drake Equation?

400

This type of planet is significantly larger than Earth but smaller than Neptune, with a thick atmosphere and potentially a rocky core.

What is a super-Earth?

400

One major limitation of the radial velocity method is that it cannot determine this orbital parameter without additional data.

What is the orbital inclination?

400

Combining the transit method with radial velocity data allows astronomers to estimate this property of the exoplanet.

What is its density (or mass and radius together)?

400

Launched in 2006, this French-led mission was the first to detect transiting exoplanets from space.

What is CoRoT (Convection, Rotation and planetary Transits)?

400

The detection of gases like oxygen, ozone, or methane in an exoplanet's atmosphere could be considered this type of evidence for life.

What is a biosignature?

500

This effect, caused by a star's motion toward and away from us, allows astronomers to detect planets via changes in the star’s spectrum.

What is the radial velocity method?

500

The minimum mass of a detected exoplanet by radial velocity is often expressed with this formulaic term.

What is M sin i (mass times sine of inclination)?

500

During transit, starlight passing through an exoplanet’s atmosphere can reveal its composition using this technique.

What is transmission spectroscopy?

500

This mission, planned by NASA, will use direct imaging to study Earth-like exoplanets around Sun-like stars.

What is the Habitable Worlds Observatory (or formerly LUVOIR/HabEx concepts)?

500

The only planet for which we have 100% evidence of life

What is Earth?