|
|
5
|
A binary star system in which one star periodically blocks the light from the other.
|
8
|
A mathematical method of writing numbers using powers of ten.
|
9
|
A galaxy shaped like a round or flattened ball, generally containing only old stars.
|
10
|
One of the small asteroid-like bodies that formed the building blocks of the planets.
|
11
|
The blue-white hot core of a star that is left behind after its outer layers have expanded and drifted out into space.
|
12
|
A mysterious force that appears to be causing the expansion of the universe to accelerate.
|
13
|
A large cloud of gas and dust in space, spread out in an immense volume.
|
15
|
A large, round, densely-packed grouping of older stars.
|
16
|
An enormously bright, distant galaxy with a giant black hole at its center.
|
17
|
The small, dense remains of a high-mass star after a supernova.
|
20
|
A galaxy with a bulge in the middle and arms that spiral outward in a pinwheel pattern.
|
22
|
A galaxy that does not have a regular shape.
|
23
|
A star cluster that has a loose, disorganized appearance and contains no more than a few thousand stars.
|
|
|
|
|
1
|
An object whose gravity is so strong that nothing, not even light, can escape.
|
2
|
A contracting cloud of gas and dust with enough mass to form a star.
|
3
|
A star system with two stars.
|
4
|
Matter that does not give off electromagnetic radiation but is quite abundant in the universe.
|
6
|
The electromagnetic radiation left over from the big bang.
|
7
|
A large cloud of gas and dust, such as the one that formed our solar system.
|
14
|
All of space and everything in it.
|
18
|
The observation that the farther away a galaxy is, the faster it is moving away.v
|
19
|
A huge group of single stars, star systems, star clusters, dust, and gas bound together by gravity.
|
21
|
The initial explosion that resulted in the formation and expansion of the universe.
|
24
|
A rapidly spinning neutron star that produces radio waves.
|
25
|
The brilliant explosion of a dying supergiant star.
|
|
|