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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. 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 _____.
We don't know. It might be but does not have to be.
Nucleus
density waves
Flat - Remain Parallel - Exactly 1
2. A star that is burning hydrogen to helium in a shell surrounding it's core
Sunspot cycle
Spectroscopic parallax
Red Giant Branch Star
Celestial Equator
3. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
nucleus
Seeing
Negative - Diverge - Less than 1
conjunction
4. Is there water on the moon?
300000 KM/sec
Dwarf planets
Yes - frozen at the poles- remains protected from the suns rays
Eyepiece Lens
5. The Greek philosopher responsible for making the stellar magnitude scale.
Occam's razor
radiant
Cassegrain Focus
Hipparchus
6. Why do Galaxies move very rapidly in the interiors of the dense clusters?
radiant
contrast northern lowlands and the southern highlands of mars...
epicycle
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
7. 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.
era of recombination
direct motion
Focal Length
Sc spiral galaxy
8. A measure of the seasonal shifting of a star's position against farther stars or galaxies. The closer the star - the greater is the angular distance it shifts. We use it to find distances to stars that are up to 1000 pc away.
Parallax
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
Umbra
Trojan asteroids
9. IO
meteoriod
self-propagating star formation
Electron
MOONS: most geologically active
10. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
Jupiters red spot
supernova
Rich Cluster
isotropic
11. Possible Fates of the Universe
Differential Rotation
Hyashi track
Red Giant Branch Star
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
12. Moon in less than the angular diameter of the Sun.
MOONS: thickest atmosphere
Nebula
Annular Eclipse
Spectroscopic parallax
13. The Greek philosopher responsible for making the stellar magnitude scale.
Hipparchus
Instability strip
Apollo asteroids
least dense
14. The surface of the sun
Dwarf planets
Light Gathering Power
Precession
Photosphere
15. 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
Electromagnetic Radiation: Gamma Ray
aphelion
Kuiper belt
16. When a planet lines up with the sun inthe sky
Blackbody Curve
Annular Eclipse
critical density
conjunction
17. A faint - remarkably uniform distribution of radiation in space
Colestial Pole
Cosmic Microwave Background
general star population
Spectroscopic Parallax
18. The number of protons in an atom.
MOONS: most geologically active
Atomic Number
radio galaxy
anorthosite
19. The normal eastward movement of a planet against the background of hte distant stars.
direct motion
Ole Roemer
Continuous Spectrum
Electromagnetic Radiation: Infrared
20. What do we think the actual fate of the universe will be and why do we think this?
CCD
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
dark energy
mare basalt
21. The gap etween saturn's A and B rings
Hyashi track
Cassini division
Granules
highlands
22. A star without enough mass to begin hydrogen fusion
Neutron Star
Electromagnetic Radiation: Gamma Ray
Brown dwarf
most eccentric orbit
23. Venus
widmanstatten pattern
hottest surface
meteoriod
solar nebula
24. A spinning neutron star
Absolute Magnitude
Metals
Pulsar
tectonics of Venus
25. 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.
Nucleus
Limb darkening
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
MOONS: larger than mercury
26. Star speed at outer edge of galaxy should begin to diminish - but they dont so we guess that this means there is increasing force (aka dark matter)
cosmic singularity
rotation curve = dark matter?
Refractor
The Local Group
27. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
Hyashi track
Most dense
HII Region
resonance
28. Jupiter
Hydrostatic Equilibrium
anorthosite
most moons
Kirkwood gaps
29. 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)
Electromagnetic Radiation: Visible Light
Make up of the jovian planets
planetary nebula
Filament
30. Half of the longest diameter across an ellipse
cosmological red shift
semimajor axis
Most dense
aphelion
31. How is the Hubble Law consistent with an expanding universe?
If it is in a denser medium - such as glass - it will move slower
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.
Cosmic Microwave Background
Main Sequence
32. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
epicycle
Quasar
thinnest atmosphere
Ole Roemer
33. The faint glow of light left over from the Big Bang. cosmic microwave background are the photons that remain after the big bang that have not turned into matter.
Io (jupiters moon)
Sb spiral galaxy
fewest moons
CMB
34. A representation of the changes in color and brightness of an evolving protostar.
cosmological red shift
Hyashi track
Big Bang
Hipparchus
35. Why does the earth have few craters while the moon has many?
Cosmic Microwave Background
widmanstatten pattern
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
radiation pressure
36. The north-south line passing directly overhead through the zenith.
Meridian
Sunspot cycle
accretion
Electromagnetic Radiation
37. Any class of objects with a uniform luminosity used to determine distance.
nova
Gravitational Lens
standard candle
Turn off Point
38. Light-colored high-pressure bands in Jupiter's atmosphere
Plank's Law
Flat - Flat
Shepherd satellite
zone
39. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
rotation curve=winding dilemma?
synchronous rotation
Electromagnetic Radiation: Gamma Ray
radio lobe
40. Titan
Dwarf planets
MOONS: thickest atmosphere
differential rotation
Gamma ray bursts
41. 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)
nucleus
quasar
Europa (Jupiters moon)
Thickest atmosphere
42. The telescope configuration that has the focus placed at the back of the primary mirror
Density Wave
Spectroscopic parallax
The Big Bang Theory
Cassegrain Focus
43. 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.
Flat - Remain Parallel - Exactly 1
Black Hole
Oort Cloud
Particle Horizon
44. 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.
Thermonuclear Fusion
tectonics of Venus
Bok Globule
Sb spiral galaxy
45. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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46. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
Turn off Point
greatest elongation
interstellar dust
Electromagnetic Radiation: Visible Light
47. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
disk
MOONS: thickest atmosphere
density waves
scarp
48. A quantity measuring the stability of the Earth's atmosphere
OB Associations
Seeing
Hipparchus
Electromagnetic Radiation: Infrared
49. A telescope that uses lenses to focus light
Refractor
Light Pollution
cosmology
Flare
50. Where is the center of the expansion
Black Hole
Electromagnetic Radiation: Visible Light
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.
Io (jupiters moon)