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Total cards: 13•Content version: v4•Public deck•Updated: 8/1/2026

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#1
Front (Question)

Give formula for finding whether a star dims or gets brighter. Explain how it works.

Back (Answer)

2.5log( F1 / F2) F1 = initial flux / brightness F2 = later flux / brightness If output is negative star became brighter. If output is positive star became dimmer.

#2
Front (Question)

If the apparent magnitude of a star at 3.6pc is 14.7, how do we find the absolute magitude. Explain how formula works.

Back (Answer)

m - M = 5log(d) - 5 where d is the distance in pc M is the absolute magnitude m is the apparent magnitude

#3
Front (Question)

Steffan bozeman law.

Back (Answer)

F = sigma * T^4

#4
Front (Question)

Three formula for stars.

Back (Answer)

L = 4 * Pi * R^2 * sigma * T^4 L = 4 * Pi * d^2 * b d = 1 / p

#5
Front (Question)

How do we calculate semi-major axis when we have perihelion and aphelion?

Back (Answer)

average distance.

#6
Front (Question)

Formula for doppler shift with wavelength.

Back (Answer)

λ ′ =λ(1− (observed speed / speed of light)) ​ ​ )

#7
Front (Question)

Redshift Formula

Back (Answer)

z = (lambda observed - lambda) / lambda

#8
Front (Question)

Formula for distance to a galaxy using hubble’s constant.

Back (Answer)

v = z * c H0 = v / d

#9
Front (Question)

Arcminutes in degrees.

Back (Answer)

1 / 60th

#10
Front (Question)

Differentiate between doppler shift and cosmological redshift.

Back (Answer)

The apparent change in frequency (and hence wavelength) of a wave due to the relative motion between the source and the observer. The increase in the wavelength of light from distant galaxies due to the expansion of the universe, caused by the stretching of space itself rather than the motion of the source.

#11
Front (Question)

Outline 3 differences between explosive nuclear processes involving white dwarfs and those involving neutron stars.

Back (Answer)

• In novae, a runaway thermonuclear reaction occurs when hydrogen is ignited. Helium ignites on neutron star surface in XRB. • In novae, visible and ultraviolet emitted. X-ray in XRB. • White dwarf can also have supernova type 1a, if the thermonuclear reaction takes place in the core. Neutron stars cannot lead to supernova.

#12
Front (Question)

Explain LIGO.

Back (Answer)

Laser Interferometer Gravitational Wave Observatory. Two perpendicular arms 4km long each form an L shape. A laser is split between the two arms, and reflected by mirrors at the end. The two lasers come back and recombine. Any change in the distance of the arms due to spacetime distortion alters the interference pattern of the lasers.

#13
Front (Question)

What is the relationship between gravitational waves and GRB?

Back (Answer)

Both are produced in cataclysmic universe events such as neutron star and black hole mergers. Gravitational waves occur as they merge, GRB occurs after.