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Test your basic knowledge |
Cosmology
Start Test
Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
If you are not ready to take this test, you can
study here
.
Match each statement with the correct term.
Don't refresh. All questions and answers are randomly picked and ordered every time you load a test.
This is a study tool. The 3 wrong answers for each question are randomly chosen from answers to other questions. So, you might find at times the answers obvious, but you will see it re-enforces your understanding as you take the test each time.
1. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
Spectral Lines
bulge
Focal Plane
Thermal Equilibrium
2. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Nova
Ammonia - methane - and water
Kirkwood gaps
Molecular Clouds
3. First accurately measured the speed of light in a vacuum
A family of radiant energy- includes light
Ole Roemer
Cepheid Variable
resonance
4. The displacement of spectral lines to redder colors caused by the expansion of the universe.
Electromagnetic Radiation: Gamma Ray
cosmological red shift
Supernova (You can be my supernova girl)
planetesimal
5. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Spectroscopic parallax
Europa (Jupiters moon)
Gravitational Lens
CNO Cycle
6. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
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7. Hydrogen and helium (mainly)
superclusters
Flat - Flat
Make up of the jovian planets
accretion disk
8. Light-colored high-pressure bands in Jupiter's atmosphere
Globular Cluster
Sa spiral galaxy
zone
Maria
9. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
tectonics of Venus
Open - flat - and closed.
Triple Alpha rocess
asteroid
10. A rock or iron specimen that has fallen from space
meteorite
meteor
Extrasolar Planet
Make up of the terrestrial planets
11. The gap etween saturn's A and B rings
tectonics of Mars
AGN
Cassini division
Trojan asteroids
12. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
accretion disk
quasar
Main Sequence Stars
meteor shower
13. The light produced when particles from the sun collide with atmospheric molecules
Electromagnetic Radiation: X-Ray
aurora
Zenith
Instability strip
14. Wave- only waves cause an interference pattern when passing through a double slit - particle- only particles deposit energy at specific locations (the way an image builds up on digital camera)
OB Associations
Parallax
Light: travels like a wave - detected like a particle
Interstellar Extinction
15. The most mass a white dwarf can have before collapsing to a neutron star
Chandrasekhar Limit
evidence of water on mars
blazar
Inverse Square Law
16. Mercury - Venus - Earth - Mars
Terrestrial Planets
planetary nebula
AGN
roche limit
17. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
terrestrial planet
quasar
gravity
Neutron Star
18. 10 nm 10^2 nm
meteoriod
Electromagnetic Radiation: X-Ray
nucleus
Filament
19. The study of the universe as a whole.
Limb darkening
cosmology
chondrite
Proton-proton chain
20. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Corona
terrestrial planet
Spectroscopic Parallax
meteorite
21. The location in the Milky Way where stars orbit like a solid wheel
Wein's Law
terrestrial planet
contrast northern lowlands and the southern highlands of mars...
Bulge
22. The temp at which a substance in the vacuum of space solidifies
Sa spiral galaxy
Cassegrain Focus
condensation temperature
Molecular Clouds
23. The state of having a balance between inward and outard pressures in a gas--the inward force from gravity is balanced by the outward force from heat.
Annular Eclipse
Hydrostatic Equilibrium
cosmological principle
Sa spiral galaxy
24. A term referring to Jupiter-like planets
meteoriod
terrestrial planet
jovian
Terrestrial Planets
25. Titan
shape and color of ELLIPTICAL galaxies
MOONS: thickest atmosphere
Vernal Equinox
Parallax
26. Why does the earth have few craters while the moon has many?
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Bok Globule
Convection
Photometry
27. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Ganymede (Jupiter)
supermassive black hole
mass
If it is in a denser medium - such as glass - it will move slower
28. When one side of a body always faces the planet it revolves around
Oort cloud
Electromagnetic Radiation: Radio
Maria
synchronous rotation
29. The particle horizon is the farthest we can see. It exists because the universe had a beginning and thus a definite age. Light from distances farther away from the particle horizon have not had time to reach us yet.
Particle Horizon
Extrasolar Planet
Electromagnetic Radiation: X-Ray
Photon
30. What causes the zones and belts on jupiter and saturn?
least dense
High and low pressure which stretch into bands due to the rapid differential rotation. deeper - darker colors are in the belts and zones are lighter
Planck time
Parallax
31. The lowest energy of an atom.
dark matter
Winter Solstice
Ground State
Electromagnetic Radiation
32. The process similar to conduction by which energy moves from the solar core to the convective layer
Radiative Diffusion
jovian
Cosmic Microwave Background (CMB)
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.
33. Venus
CNO Cycle
Plank's Law
Thickest atmosphere
CMB
34. Large nebula consisting of very cold gas and dust
Metals
Molecular Clouds
Neutron Star
Plague
35. Extends to a distance of 50000AU. Same objects as in the Kuiper belt-when they fall in toward the sun they become comets. Debris from comets hitting the Earths atmosphere cause meteor showers.
White Dwarf
Color Index
Oort Cloud
Extrasolar Planet
36. The imaginary sphere centered on the Earth that hols the stars.
Celestial Sphere
Summer Solstice
Hipparchus
greehouse effects
37. The number of protons in an atom.
Bok Globule
superclusters
Atomic Number
epicycle
38. A word used in astronomy to describe all elements besides hydrogen and helium
Metals
synchrotron radiation
Thermal Equilibrium
Black Hole
39. A galaxy emitting large amounts of energy at long wavelengths.
Dark matter candidates
general star population
deferent
radio galaxy
40. The oldest terrain on the moon
Cosmological Principle
highlands
Heliocentric
density parameter
41. When massive objects bend space and time enough to create multiple images of an object located behind them
inferior planets
deferent
Focal Plane
Gravitational Lens
42. An entity that is likely in the nucleus of most - if not all - galaxies.
cosmic fireball
Photosphere
supermassive black hole
Rich Cluster
43. The place in the sky that the Earth's axis points toward (can be either north or south)
Colestial Pole
widmanstatten pattern
SETI
Hipparchus
44. The elementary building blocks from which protons and neutrons are formed.
molecular clouds
Ole Roemer
Cepheid Variable
quarks
45. A huge sphere of tenuous gas surrounding the nucleus of a comet
Globular Cluster
coma
synchronous rotation
Stephen-Boltzman Law
46. The relation that tells how light dims with distance.
shape and color of SPIRAL galaxies
critical density
Limb darkening
Inverse Square Law
47. Flat disk with gas - dust - H2 regions - molecular clouds - dust young stars and remnants of old planetary nebula and supernova remnants. stars spin together with similar velocities called differential rotation
Resolving Power
CMB
disk
Supernova (You can be my supernova girl)
48. Dying small mass stars lose their outer layers in a relatively gentle way - creating a round or bipolar nebula about the star (round like planets)
planetary nebula
blazar
AGN
Dark Nebula
49. The wavelengths where a specific element can absorb or emit light.
Planetary Nebula
Spectral Lines
synchronous rotation
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
50. A star that blows itself apart
Supernova (You can be my supernova girl)
Gamma-ray Burst
Lagrangian Razor
self-propagating star formation