Blackbody Radiation
Cosmology
Celestial Mechanics
More Celestial Mechanics
Trivia
100

This is the term for an object that absorbs all radiation incident on it and emits radiation based on its temperature.

What is a blackbody?

100

This is the name of the theory that describes the origin of the universe as a rapid expansion from a singularity.

What is the Big Bang Theory?

100

This law states that the square of the orbital period of a planet is proportional to the cube of the semi-major axis of its orbit.

What is Kepler's Third Law?

100

This equation describes the gravitational force between two masses, m1 and m2, separated by a distance r.

What is Newton's Law of Gravitation (F = Gm1m1/r2)?

100

Solar luminosity relates to distance in this way.

What is the inverse-square law?
200

This law states that the wavelength at which a blackbody emits the most radiation, given by λmax=b/T

What is Wien's Displacement Law?

200

This is the apparent shift in the position of an object when viewed from two different locations.

What is parallax?

200

This is the process by which the Moon's gravitational pull creates two bulges on Earth's liquid surface.

What is tidal force?

200

This is the term for the point in a system where the gravitational force acts as if all the mass were concentrated.

What is the center of mass?

200

Although the Sun appears yellow from Earth, this is its true color when observed from space, due to its blackbody radiation curve peaking in this part of the visible spectrum.

What is white?

300

This formula relates a star's luminosity, radius and temperature: L = 4πR2σT4

What is the Stefan-Boltzmann Law?

300

This is the unit of distance used in astronomy, defined as the distance at which a star would have a parallax of 1 arcsecond.

What is a parsec?

300

These are points in a two-body system where a third object can remain in a stable position relative to the two larger bodies.

What are Lagrange points?

300

This is the value of the gravitational constant (G) in SI units.

What is 6.674×10−11N⋅m2/kg2?

300

This is the name of a group of old stars closely packed in symmetrical form.

What is a Globular Star Cluster?

400

As a blackbody's temperature increases, the peak wavelength of its emitted radiation approaches the end of the visible spectrum into this color

What is Blue/Violet?

400

The accelerating expansion of the universe is attributed to this mysterious force.

What is Dark Energy?
400

This formula calculates the escape velocity from the surface of a planet, where G is the gravitational constant, M is the planet's mass, and r is its radius.

What is v = sqrt(2GM/r)?

400

This distance from a celestial body marks the point where its gravitational pull overcomes the force keeping an object together.

What is the Roche Limit?

400
The sun periodically discharges these from its corona.
What are Coronal Mass Ejections (CMEs)?
500

This is the name of the curve that describes the intensity of radiation emitted by a blackbody at different wavelengths.

What is the Planck curve?

500

This is the observed redshift of distant galaxies, which provides evidence for the expansion of the universe.

What is Hubble's Law?

500

This is the formula for the spherical law of cosines, relating the sides (a,b,c) and angles (A,B,C) of a spherical triangle.

What is cos⁡(a) = cos⁡(b)cos⁡(c)+sin⁡(b)sin⁡(c)cos⁡(A)?

500

This is the gravitational potential energy formula for two masses separated by a distance r.

What is U = −Gm1m2/r?

500

This layer of the sun may be seen with the naked eye.

What is the Photosphere?

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