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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. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
density
We don't know. It might be but does not have to be.
Dark Nebula
tectonics of Earth
2. Jupiter
MOONS: thickest atmosphere
difference between maria and highlands of the moon.
Kuiper belt
most moons
3. The name for the only seriously considered theory of the universe.
Gamma ray bursts
E=mc2
Big Bang
Differential Rotation
4. Where is the center of the expansion
Cosmological Principle
Enke gap
How is winding dilemma solved?
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.
5. The light produced when particles from the sun collide with atmospheric molecules
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
aurora
density
radio galaxy
6. A word used in astronomy to describe all elements besides hydrogen and helium
standard candle
thinnest atmosphere
Electromagnetic Radiation
Metals
7. 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
Annular Eclipse
Light-Year
Thermal Equilibrium
Hubble law
8. A faint - remarkably uniform distribution of radiation in space
Atomic Number
Cosmic Microwave Background
quarks
Planck time
9. 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.
Refractor
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Limb darkening
Differential Rotation
10. Small moons that maintain the shape of rings around Saturn and Uranus
planetary nebula
Shepherd satellite
Light-Year
Grand design spirals
11. 1 mm 1μm
Main Sequence Stars
Electromagnetic Radiation: Infrared
Red Giant
Celestial Sphere
12. The amount an image is enlarged by a telescope
self-propagating star formation
Magnification
OB Associations
partile horizon
13. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
supernova
Stephen-Boltzman Law
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Primary Mirror
14. An energetic event taking place in the early universe
Astronomical Unit
Gamma-ray Burst
Sa spiral galaxy
zone
15. A star without enough mass to begin hydrogen fusion
Supercluster
radiation dominated universe
Bok Globule
Brown dwarf
16. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
radiation dominated universe
Positive - Converge - Greater than 1
Active Optics
Ionization
17. 10^2 nm 10^7 nm
planetary nebula
Electromagnetic Radiation: Gamma Ray
It does not have to expand into anything. It might just be that the 3 dimensions of space are getting bigger. It may also be that our 3 spatial dimensions are expanding into higher dimensions if such things exist.
Cassegrain Focus
18. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
Continuous Spectrum
opposition
dark energy
Spectroscopic parallax
19. A location on an H-are Diagram where evolving stars pulsate
Instability strip
Galilean satellite
slowest rotation
Electromagnetic Radiation: Ultraviolet Light
20. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
Poor Cluster
Light-Year
High Velocity Stars
Cosmic Microwave Background (CMB)
21. 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)
H2 Regions
Open - flat - and closed.
Rich Cluster
Metals
22. 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.
Lagrangian Razor
radio galaxy
difference between maria and highlands of the moon.
contrast northern lowlands and the southern highlands of mars...
23. A measure of the ability of a telescope to see fine detail
synchronous rotation
Resolving Power
Main Sequence
Galilean satellite
24. Ganymede and Titan
Objective Lens
disk
MOONS: larger than mercury
Flare
25. Long - meandering cliff formed when a planet surface cools and shrinks
Nucleus
Coronal Loop
The Big Bang Theory resolves Olber's Paradox
scarp
26. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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27. A small spherical dark nebula
Astronomical Unit
Total Eclipse
Bok Globule
Self-Propogating Star Formation
28. A small chunk of rock in space
Supercluster
radiation pressure
meteoriod
accretion disk
29. How is the Hubble Law consistent with an expanding universe?
great dark spots
Refractor
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.
Flocculent spirals
30. The apparent backward motion of a planet against the background of stars.
Disk
retrograde motion
Ganymede (Jupiter)
Gamma ray bursts
31. A change in the appearance of the sun at the edge of the solar disk
Light Pollution
Electromagnetic Radiation: Gamma Ray
condensation temperature
Limb darkening
32. A term referring to Earth-like planets
The Big Bang Theory resolves Olber's Paradox
Electromagnetic Radiation
terrestrial planet
open star clusters
33. A long-lived high-pressure bulge in Jupiter's southern hemisphere
Most dense
Radio Galaxy
great red spot
Vernal Equinox
34. The shadow behind the Earth or Moon where the Sun is partially obscured.
Thickest atmosphere
Pulsar
Penumbra
Gamma-ray Burst
35. Where is the center of the expansion
Prominence
Jupiters red spot
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.
Jovian Planets
36. VENUS
Geocentric
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
Gamma-ray Burst
Metals
37. A particle of light
Cassini division
dark energy
Electromagnetic Radiation
Photon
38. Theory virtually demands that the geometry of the universe be ______. Results of measuring lumps in the cosmic background radiation indicate that the universe geometry is ________.
Absorption Spectrum
Bok Globule
roche limit
Flat - Flat
39. A crystalline patter found in iron meteorites
widmanstatten pattern
Plague
Olber's paradox
rotation curve=winding dilemma?
40. A rock or iron specimen that has fallen from space
Supercluster
Electromagnetic Radiation: Infrared
meteorite
rotation curve = dark matter?
41. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
slowest rotation
tectonics of Mars
Extrasolar Planet
accretion disk
42. 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 _____.
protostar
Flat - Remain Parallel - Exactly 1
slowest rotation
Electromagnetic Radiation: Infrared
43. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
standard candle
Spectroscopic Parallax
Ole Roemer
Gamma ray bursts
44. The name for the only seriously considered theory of the universe.
3 reasons we orbit satellites to observe universe
We don't know. It might be but does not have to be.
Big Bang
Nebula
45. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
Electromagnetic Radiation: Gamma Ray
shape and color of SPIRAL galaxies
Halo
density parameter
46. A distance measure determined by the shifting of a star against the background sky every 6 months.
Filament
H-are Diagram
Autumnal Equinox
Parsec
47. The rate of expansion of the universe.
tectonics of Venus
great dark spots
How is winding dilemma solved?
Hubble constant
48. A huge sphere of tenuous gas surrounding the nucleus of a comet
weight
Main Sequence
coma
Black Hole
49. The equation that describes how matter equates with energy
Limb darkening
E=mc2
quarks
Parallax
50. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
Instability strip
CCD
Total Eclipse
Disk