TYPES OF GALAXIES
STARS
LIFE STAGES
TERMINOLOGIES
PROPERTIES OF STARS
100

the galaxy our sun lives in

MILKY WAY GALAXY

100

huge, massive spheres of incandescent gas much like our sun

STARS

100

a large cloud of gas or dust in space

NEBULA

100

a group of stars forming a recognizable pattern that is traditionally named after its apparent form or identified with a mythological figure

CONSTELLATIONS

100

super giant, giant, and dwarf


SIZE

200

look like thin lenses or whirlpools

SPIRAL

200

biggest star in our solar system

SUN
200

exerts such a strong gravitational pull that no light escapes

BLACKHOLE

200

reaction in which two or more nuclei are combined to form one or more different atomic nuclei and subatomic particles

NUCLEAR FUSION

200

brightness of stars

MAGNITUDE

300

flat, circular or ellipsoidal shapes resembling the central disk of spiral galaxies

ELLIPTICAL

300

graph showing the relationship between luminosity and temperature

H-R DIAGRAM

300

the earliest stage of a star's life

PROTOSTAR

300

distance that light travels in one year which is equal to 9.46 trillion kilometers

LIGHT YEAR

300

amount of light emitted by an object in a unit of time

LUMINOSITY

400

lack definite shape or symmetry, large and small magellanic clouds belong to this type

IRREGULAR

400

star closest to our sun, has a parallax of about 0.76 second

PROXIMA CENTAURI

400

 

a celestial object of very small radius (typically 18 miles/30 km) and very high density, composed predominantly of closely packed neutrons,  thought to form by the gravitational collapse of the remnant of a massive star after a supernova explosion


NEUTRON STAR

400

a measure of how bright a star appears to be on earth

APPARENT MAGNITUDE

400

the color of stars depend on differences in this rather than in composition

TEMPERATURE

500

slightly farther at 180,000 light years away, it is situated at the south celestial  pole near the constellation Tucana

SMALL MAGELLANIC CLOUDS

500

a Greek astronomer, introduced a scheme of classifying stars according to their apparent magnitude

HIPPARCHUS

500

about 90 percent of the stars in the universe, including the sun, these stars can range from about a tenth of the mass of the sun to up to 200 times as massive.

MAIN SEQUENCE STAR

500

A change in an object’s direction due to a change in the observer’s position

PARALLAX

500

a  measure of how bright a star would be if all stars were at the same distance

ABSOLUTE MAGNITUDE

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