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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. 1. We see rapid movements or high energy radiation coming at some level from the nuclei of nearly every galaxy we have looked at. 2. We suspect that the creation of these supermassive black holes is part of the galaxy formation process.
molecular clouds
Olber's paradox
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
2. The material from which the solar system formed
Population 1 vs Population 2 stars
Hubble law
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.
solar nebula
3. 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)
Photon
Chromosphere
matter dominated universe
great dark spots
4. Light scattered through the atmosphere that degrades astronomical images
Light Pollution
MOONS: thickest atmosphere
300000 KM/sec
Proton-proton chain
5. A faint - remarkably uniform distribution of radiation in space
Stephen-Boltzman Law
Coldest surface
OB Associations
Cosmic Microwave Background
6. The imaginary sphere centered on the Earth that hols the stars.
quasar
planetary nebula
Celestial Sphere
Sc spiral galaxy
7. The rock that makes up the lunar highlands
SETI
anorthosite
Electromagnetic Radiation: Infrared
Kuiper belt
8. A high-pressure bulge in Neptune's southern hemisphere
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Vernal Equinox
Light Gathering Power
great dark spots
9. When the Moon entirely blocks the Sun.
Apparent Magnitude
Total Eclipse
Interstellar Extinction
MOONS: thickest atmosphere
10. A phenomenon seen when the Earth passes through the orbit of a burned out comet
MOONS: larger than mercury
self-propagating star formation
meteor shower
The Big Bang Theory resolves Olber's Paradox
11. 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.
highlands
Eclipses of the Moons of Jupiter
Callisto (Jupiter)
12. The projection of the Earth's equator onto the celestial sphere.
Disk
Celestial Equator
HII Region
fewest moons
13. Electromagnetic Radiation
Disk
Electromagnetic Radiation: Microwave
Reflector
A family of radiant energy- includes light
14. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
Absorption Spectrum
Neutron Star
Io (jupiters moon)
15. The gap inthe outer portion of Saturn's A ring
meteor shower
Enke gap
Rich Cluster
MOONS: larger than mercury
16. The Big Bang was not an explosion of matter into empty space - like the explosion of a bomb. Instead - it was an emergence of space and time filled with pure energy where before none of this was present. The point from which is emerged is called the
supermassive black hole
Sidereal Day
The Big Bang Theory
force
17. A small round distribution of gas surrounding a dying star
Nova
Dark Nebula
Planetary Nebula
contrast northern lowlands and the southern highlands of mars...
18. The lens in a telescope used to determine the magnification
Maria
Rich Cluster
Make up of the jovian planets
Eyepiece Lens
19. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
Disk
Total Eclipse
density waves
Flat - Flat
20. A term referring to the orbital character of stars near the Sun
comet
Penumbra
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.
Differential Rotation
21. When material is heated and moves taking the heat energy with it
Convection
Oort cloud
SETI
meteor
22. 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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23. A measure of the ability of a telescope to see fine detail
Thickest atmosphere
Supercluster
Resolving Power
density
24. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
disk
Negative - Diverge - Less than 1
CMB
Dark Matter
25. The organization of clusters of galaxies into sheets and strings
Galilean satellite
Supercluster
anorthosite
superclusters
26. The displacement of spectral lines to redder colors caused by the expansion of the universe.
tectonics of Mars
dark matter
cosmological red shift
Most dense
27. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Celestial Sphere
Particle Horizon
molecular clouds
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
28. The organization of clusters of galaxies into sheets and strings
Hydrostatic Equilibrium
Supercluster
Make up of the terrestrial planets
Interstellar Extinction
29. The time when the universe cooled sufficiently for atoms to exist. radiation dominated= first 300000 years - THEN era of recombination turns into matter dominated for next.
great red spot
The Local Group
Absolute Magnitude
era of recombination
30. 10 nm 10^2 nm
Plague
Callisto (Jupiter)
Flocculent spirals
Electromagnetic Radiation: X-Ray
31. In what chemical form are jupiters nitrogen - carbon and oxygen?
matter dominated universe
Drake equation
Poor Cluster
Ammonia - methane - and water
32. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Terrestrial Planets
synchrotron radiation
Grand design spirals
molecular clouds
33. Centered on the Earth
Atomic Number
great red spot
Geocentric
Open Cluster
34. The light produced when particles from the sun collide with atmospheric molecules
Doppler Shift
evidence of water on mars
aurora
accretion
35. 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.
partile horizon
tectonics of Venus
Gravitational Lens
OB Associations
36. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Open - flat - and closed.
Light-Year
isotropic
Callisto (Jupiter)
37. An empirical scheme for predictin ghe orbital distances of planets
Pulsar
nucleus
Titus-Bode Law
Black Hole
38. A huge sphere of tenuous gas surrounding the nucleus of a comet
coma
Energy Level
MOONS: thickest atmosphere
Radio Galaxy
39. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
Seyfert galaxy
Flocculent spirals
Sunspots
opposition
40. Venus
MOONS: thickest atmosphere
jovian
Kirchhoff's Law
Thickest atmosphere
41. Approximate speed of light in a vacuum
Electromagnetic Radiation
Supercluster
300000 KM/sec
zone
42. A long-lived high-pressure bulge in Jupiter's southern hemisphere
The Big Bang Theory resolves Olber's Paradox
great red spot
blazar
Spectral Lines
43. Distribution of dust (tells us disk is thin) - find distances to O&B stars and H2 regions (arms are sights of star formation and OB stars live and die at location of birth) -Milky way has four arms. Sun is in spur apart from arms.
mapping the structure of Milky Way disk
Active Optics
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.
Supernova (You can be my supernova girl)
44. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
quasar
Hubble law
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.
MOONS: larger than mercury
45. The rate of expansion of the universe.
Secondary Mirror
Hubble constant
Autumnal Equinox
Oort cloud
46. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
CNO Cycle
Secondary Mirror
MOONS: larger than mercury
Halo
47. When the Sun is farthest south of the celestial equator (About December 22)
greatest elongation
Parallax
Winter Solstice
planetary nebula
48. A particle of light
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
density
meteor shower
Photon
49. The mass of an object divided by its volume
most moons
Ecliptic
chondrite
density
50. The material from which the solar system formed
Flare
solar nebula
Focal Length
Radiative Diffusion