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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. The relation that tells how light dims with distance.
Resolving Power
interstellar dust
Inverse Square Law
Objective Lens
2. The name for the only seriously considered theory of the universe.
Kirchhoff's Law
Supercluster
Yes - frozen at the poles- remains protected from the suns rays
Big Bang
3. Venus
hottest surface
Pulsar
Globular Cluster
chemical differentiation
4. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
dark energy
Sb spiral galaxy
Winter Solstice
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
5. Venus (retrograde)
Coldest surface
slowest rotation
Superior planets
Milky way Galaxy
6. Long - meandering cliff formed when a planet surface cools and shrinks
Light Gathering Power
scarp
Parallax
gravity
7. Any change in the speed or direction of an object's motion
acceleration
Trojan asteroids
scarp
bulge
8. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Main Sequence Stars
quarks
Spectroscopic Parallax
critical density
9. A small round distribution of gas surrounding a dying star
Annular Eclipse
Planetary Nebula
tectonics of Venus
great dark spots
10. 10 cm -> 1 mm
Electromagnetic Radiation: Microwave
mass
opposition
Supernova (You can be my supernova girl)
11. A star that is burning hydrogen to helium in a shell surrounding it's core
Pulsar
Penumbra
Red Giant Branch Star
Electromagnetic Radiation
12. The number of protons in an atom.
Titus-Bode Law
Milky way Galaxy
Atomic Number
direct motion
13. An element of a highly efficient - two-dimensional electronic light detector
Pixel
Vernal Equinox
jovian
Main Sequence Stars
14. After stars form they pump light energy into surrounding gas causing it to heat up and glow (H2=ionized hydrogen - H1= neutral hydrogen in molcular couds)
nucleus
greatest elongation
Focal Length
H2 Regions
15. The most mass a white dwarf can have before collapsing to a neutron star
MOONS: roundest shape
Objective Lens
Chandrasekhar Limit
Spectral Lines
16. Matter that reveals itself only through its gravitational attraction
Dark Matter
Kirkwood gaps
anorthosite
Coldest surface
17. Where is the center of the expansion
neutrino
Neutron Star
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
Sa spiral galaxy
18. The movement of the Earth's crustal plates riding on top of the mantle.
Flare
terrestrial planet
cosmological red shift
plate tectonics
19. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
Light: travels like a wave - detected like a particle
neutrino
Electromagnetic Radiation: X-Ray
direct motion
20. The mirror that gathers the light in a reflector
Primary Mirror
cosmic fireball
cosmology
Trojan asteroids
21. When one side of a body always faces the planet it revolves around
synchronous rotation
Titus-Bode Law
Electromagnetic Radiation: Radio
Photon
22. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
aurora
Halo
Supernova (You can be my supernova girl)
self-propagating star formation
23. A force exerted by reflecting sunlight
Cosmological Principle
radiation pressure
cosmological red shift
Plague
24. 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.
Hydrostatic Equilibrium
MOONS: thickest atmosphere
Parsec
cosmological principle
25. A planet that is closer to the sun than the earth
retrograde motion
hottest surface
inferior planets
Light Gathering Power
26. IO
slowest rotation
MOONS: most geologically active
Kuiper belt
Emission Spectrum
27. The mass of an object divided by its volume
density
CMB
great dark spots
Astronomical Unit
28. The lens that gathers the light in a refractor
greehouse effects
critical density
Objective Lens
Chromosphere
29. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
self-propagating star formation
CNO Cycle
Open Cluster
chondrite
30. The family of radiant energy that includes light as a subset
synchronous rotation
Absorption Spectrum
Electromagnetic Radiation
Parsec
31. The wavelengths where a specific element can absorb or emit light.
MOONS: roundest shape
radiation pressure
Chandrasekhar Limit
Spectral Lines
32. A particle of light.
most eccentric orbit
asteroid
Photon
H2 Regions
33. N=are*Fp(Ne)(Fl)(Fi)(Fc)(L) N: number of civilizations possible to communicate with are*: rate solar-like stars are created Fp: fraction of stars with planets Ne: number of planets like ours Fl: fraction of planets with life Fi: intelligent life Fc:
Black Hole
quasar
Drake equation
Focal Plane
34. A point in the sky where meteors appear to come from during a shower
synchronous rotation
radiant
cosmological red shift
Kirchhoff's Law
35. The oldest part of the Milky Way
Filament
Cosmic Microwave Background
Halo
Cassini division
36. An object that may remain after a star explodes
300000 KM/sec
SETI
Neutron Star
Ammonia - methane - and water
37. A fusion process in which protons build together to form helium
Proton-proton chain
planetesimal
Focal Plane
aurora
38. How is the Hubble Law consistent with an expanding universe?
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.
Triple Alpha rocess
plate tectonics
Plank's Law
39. 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)
Dark matter candidates
Light: travels like a wave - detected like a particle
H-are Diagram
Quasar
40. A galaxy emitting large amounts of energy at long wavelengths.
bulge
radio galaxy
aurora
H-are Diagram
41. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
tectonics of Venus
Self-Propogating Star Formation
Winter Solstice
deferent
42. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
MOONS: roundest shape
Density Wave
critical density
Jupiters red spot
43. Originially thought to be stars emitting radio radiation but are now concluded to be nuclei of distant galaxies (same as radio galaxies aka emit streams of material)
synchrotron radiation
The Big Bang Theory
quasar
Electromagnetic Radiation
44. Collections of young - hot stars
Differential Rotation
Wein's Law
Cepheid Variable
OB Associations
45. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
The Local Group
zone
chemical differentiation
inferior planets
46. 1μm 100 nm
supernova
meteor
planetary nebula
Electromagnetic Radiation: Visible Light
47. A word meaning 'the same in all directions.'
Maria
isotropic
Sa spiral galaxy
anorthosite
48. The part of the Milky way that has on-going star formation
Disk
reflection star clusters
Synodic Day
Sa spiral galaxy
49. The area behind a lens where images are resolved
Energy Level
Focal Plane
nova
fusion crust
50. A faint - remarkably uniform distribution of radiation in space
planetesimal
Cosmic Microwave Background
Callisto (Jupiter)
Neutron Star