Space Flashcards

Get gud at space

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1
Q

Red Giant

A

a large star cooler than our sun, e.g. 3000k

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2
Q

White dwarf

A

Small hot star, e.g. 10000k

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3
Q

Blue supergiant

A

very large very hot star, e.g. 25000k

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4
Q

luminosity

A

the rate at which energy of all types is radiated by an object in all directions, measured in watts

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5
Q

Stefan-Boltzmann law

A

the power output of a black body is proportional to its surface area and the fourth power of its temperature in Kelvin, L=σAT^4

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6
Q

Wein’s Law

A

that the relationship between the peak output wavelength and temperature for a black body radiator is given by the equation λmaxT=2.898*10^-3mK

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7
Q

Hurtzsprung-Russell diagram

A

a plot of stars showing luminosity/absolute magnitude on the y-axis and temperature/spectral class on the x-axis

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8
Q

main sequence

A

a rough diagonal line from top left to bottom right of a Hurtzsprung-Russell diagram which marks stars that are in a generally stable phase in their existence

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9
Q

protostar

A

dust and gas clumping together under the force of gravity, prior to the start of nuclear fusion in its core, which will go on to become a star

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10
Q

neutron star

A

one of the possible conclusions to the life of a large mass star, small and very dense, composed of neutrons

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11
Q

black hole

A

one of the possible conclusions to the life of a large mass star, a region of space-time in which gravity is so strong that it prevents anything from escaping, including EM radiation

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12
Q

planetary nebula

A

the remnants of an explosion at the end of the life cycle of a low-mass star; material which may eventually agglomerate into new planets

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13
Q

black dwarf

A

the final stage of the life cycle of a small mass star, when nuclear fusion has ceased and it has cooled so that it no longer emits visible light

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14
Q

supernova

A

the explosion of a large mass star at the end of its lifetime, when it becomes extremely unstable

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15
Q

light year

A

the distance light can travel in one year, which is about 10^16 m

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16
Q

astronomical unit (AU)

A

the radius of the earth’s orbit around the sun; 1 AU = 1.5*10^11

17
Q

Trig parallax

A

a method for measuring the distance to relatively close stars. it works by comparing their measured angle in the sky at six-month intervals and using these measurements to calculate the distance using trigonometry

18
Q

Parallax angle

A

the difference in angular observation of a given star, for use in the trigonometric parallax method of measuring the distance to a star

19
Q

parsec (pc)

A

the distance a star must be from the sun in order for the parallax angle Earth-Star-Sun to be 1 arcsecond. 1pc = 3.09*10^16 m = 3.27 light years

20
Q

Standard candles

A

stars with properties which mean their luminosity can be determined from measurements other than apparent brightness

21
Q

redshift

A

the shift in wavelength of a star’s spectrum caused by increased separation between the star and earth

22
Q

The Doppler effect

A

when an observer receiving waves emitted from a moving body observes that the wavelength of the waves has been altered to a new wavelength as a consequence to the relative motion

23
Q

Hubble’s law

A

that the recession velocity of a galaxy is directly proportional to the distance to it

24
Q

Hubble constant

A

the constant of proportionality in Hubble’s law; H(0) = 70.9 km/s/Mpc

25
Q

Big Bang

A

the theory that the universe expanded outwards from a single point to the currently observed situation

26
Q

The Big Crunch

A

a possible future for the universe in which it contracts inwards to a single point

27
Q

Dark Matter

A

a material in the universe that explains some anomalous behaviors of celestial objects; as yet its nature has not been identified.

28
Q

Dark energy

A

a source of a force that is causing the expansion of the universe to accelerate; as yet it’s nature has not been identified