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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 average distance between the Earth and the Sun (=1.5 x10^8km)
chemical differentiation
rotation curve = dark matter?
MOONS: larger than mercury
Astronomical Unit
2. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
CNO Cycle
density parameter
Light: travels like a wave - detected like a particle
partile horizon
3. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Density Wave
greehouse effects
epicycle
4. Sc galaxies
scarp
mass
Apollo asteroids
Flocculent spirals
5. A phenomenon seen when the Earth passes through the orbit of a burned out comet
Lagrangian Razor
MOONS: roundest shape
meteor shower
era of recombination
6. Mercury - Venus - Earth - Mars
Particle Horizon
Terrestrial Planets
blazar
Hydrostatic Equilibrium
7. Venus
Roundest orbit
Summer Solstice
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
resonance
8. A planet that is farther from the sun than the Earth is
Spectral Lines
Superior planets
matter dominated universe
Sunspots
9. Titan
MOONS: thickest atmosphere
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
SETI
widmanstatten pattern
10. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
zone
direct motion
Triple Alpha rocess
epicycle
11. The process of acquiring material
cosmological principle
accretion
Ecliptic
mapping the structure of Milky Way disk
12. Is there water on the moon?
Yes - frozen at the poles- remains protected from the suns rays
cosmic singularity
Hubble constant
Electromagnetic Radiation: Visible Light
13. A telescope that uses mirrors to focus light
Oort Cloud
Reflector
Thermonuclear Fusion
Neutron Star
14. Mercury
radio lobe
thinnest atmosphere
Cepheid Variable
open star clusters
15. The crust of a meteorite caused by its entry into Earth's atmosphere
planetary nebula
The Big Bang Theory resolves Olber's Paradox
fusion crust
density waves
16. The mix of pure photon energy that emerged at the start of the universe.
rotation curve = dark matter?
cosmic fireball
Bulge
thinnest atmosphere
17. The location around an atom where an electron resides.
Energy Level
greehouse effects
Nebula
Eyepiece Lens
18. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
comet
Gamma ray bursts
fastest rotation
Jupiters red spot
19. A bridge of material held in position above the solar surface. They can remain for hours even days
tectonics of Earth
Prominence
Refractor
300000 KM/sec
20. A planet that is closer to the sun than the earth
Ammonia - methane - and water
coma
supermassive black hole
inferior planets
21. 10 nm 10^2 nm
Kuiper belt
Electromagnetic Radiation: X-Ray
Spectroscopic Parallax
Occam's razor
22. The mass of an object divided by its volume
density
resonance
coma
Proton-proton chain
23. A word meaning 'the same everywhere throughout.'
homogeneous
weight
Synchrotron Rotation
difference between maria and highlands of the moon.
24. The first rock-sized bodies that formed in the solar nebula from dust grains
Kuiper belt
chondrite
MOONS: larger than mercury
Seyfert galaxy
25. The displacement of spectral lines to redder colors caused by the expansion of the universe.
Ecliptic
Electromagnetic Radiation: Infrared
Halo
cosmological red shift
26. A small chunk of rock in space
CMB
Dark matter candidates
Limb darkening
meteoriod
27. A spinning neutron star
Blackbody
Hubble constant
Pulsar
Parsec
28. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
nova
interstellar dust
Spectroscopy
resonance
29. Either Io -Europa - Ganymede - or Callisto
Coronal Loop
Cepheid Variable
Drake equation
Galilean satellite
30. 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.
A family of radiant energy- includes light
jovian
Oort Cloud
Parsec
31. A planet that is closer to the sun than the earth
Brown dwarf
radio galaxy
inferior planets
Electromagnetic Radiation: Gamma Ray
32. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
superclusters
Ecliptic
Instability strip
Grand design spirals
33. A faint - remarkably uniform distribution of radiation in space
Winter Solstice
Cosmic Microwave Background
quarks
fewest moons
34. The point directly overhead.
mapping the structure of Milky Way disk
fusion crust
Zenith
roche limit
35. VENUS
chondrite
Clouds of sufuric acid (very inhospitable and brightest object in the sky) - process called greenhouse affect traps radiation making it 900 degrees at times - spins with retrograde rotation (sun rises in west) and takes 58.4 days for it to set. Thick
greehouse effects
Energy Level
36. A prominence seen against the disk of the sun
aurora
anorthosite
Filament
Nebula
37. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Plague
Parallax
The Big Bang Theory
Quasar
38. The gap etween saturn's A and B rings
Focal Length
Cassini division
Winter Solstice
Umbra
39. In a FLAT UNIVERSE(our universe) - the curvature of space-time is ________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
Flat - Remain Parallel - Exactly 1
greatest elongation
cosmic singularity
contrast northern lowlands and the southern highlands of mars...
40. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Halo
Milky way Galaxy
mare basalt
Electron
41. The temp at which a substance in the vacuum of space solidifies
Brown dwarf
slowest rotation
condensation temperature
Sa spiral galaxy
42. Norhern lowlands- darker in color and have far fewer craters as if an ancient sea or ice field covered them. southern highlands- much higher in density of craters.
contrast northern lowlands and the southern highlands of mars...
Plank's Law
meteor shower
Photon
43. The rate of expansion of the universe.
Hubble constant
open star clusters
Prominence
Density Wave
44. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Horizontal Branch Star
cosmological principle
Clouds of sufuric acid (very inhospitable and brightest object in the sky) - process called greenhouse affect traps radiation making it 900 degrees at times - spins with retrograde rotation (sun rises in west) and takes 58.4 days for it to set. Thick
Photometry
45. The era when the ratio of matter to energy greatly favored matter. (verses radiation dominated universe where it was opaque. Matter is now dominated by gravity not photons)
matter dominated universe
planetesimal
asteroid
resonance
46. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
reflection star clusters
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
CCD
Drake equation
47. The larger bodies that formed early in teh solar nebula that were chemically differentiated
Brown dwarf
Yes - frozen at the poles- remains protected from the suns rays
Apollo asteroids
planetesimal
48. Where is the center of the expansion
Electromagnetic Radiation: Microwave
evidence of water on mars
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.
blazar
49. A spread of light with an uninterrupted wavelength distribution of energy.
We don't know. It might be but does not have to be.
The Big Bang Theory
Cosmic Microwave Background
Continuous Spectrum
50. The elementary building blocks from which protons and neutrons are formed.
quarks
Parallax
Extrasolar Planet
Ecliptic