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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. Mercury and venus
fewest moons
Hipparchus
3 reasons we orbit satellites to observe universe
Jovian Planets
2. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
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
H2 Regions
Big Crunch
Cepheid Variable
3. 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.
Lagrangian Razor
zone
Black Hole
era of recombination
4. Earth
tectonics of Mars
Open - flat - and closed.
Most dense
Io (jupiters moon)
5. A particle of light
Apparent Magnitude
Photon
chemical differentiation
Electron
6. The rate of expansion of the universe.
Red Giant
Light Pollution
Penumbra
Hubble constant
7. Venus
Flocculent spirals
Energy Level
Planck time
hottest surface
8. The location in an H-are diagram of a star cluster - where stars have just left the main sequence. Used to estimate the cluster age.
smallest diameter
Turn off Point
Penumbra
plate tectonics
9. The powdered stone fragments that make up the lunar 'soil'
Largest diameter
Spectroscopic parallax
regolith
Continuous Spectrum
10. Titan
tectonics of Earth
Kirkwood gaps
MOONS: thickest atmosphere
Focal Length
11. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Spectroscopic Parallax
Sidereal Day
standard candle
Autumnal Equinox
12. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Gamma-ray Burst
Gravitational Lens
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
Sc spiral galaxy
13. The projection of the Earth's equator onto the celestial sphere.
Celestial Equator
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
Radiative Diffusion
Proton-proton chain
14. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Reflector
Dark Nebula
synchrotron radiation
great red spot
15. 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 _____.
Gamma-ray Burst
Black Hole
Flat - Remain Parallel - Exactly 1
Photon
16. How did Earth come to have an oxygen rich atmosphere?
Grand design spirals
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
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
most moons
17. A bridge of material held in position above the solar surface. They can remain for hours even days
Sunspot cycle
roche limit
Prominence
Black Hole
18. The larger bodies that formed early in teh solar nebula that were chemically differentiated
standard candle
Hipparchus
planetesimal
Energy Level
19. A long-lived high-pressure bulge in Jupiter's southern hemisphere
Penumbra
Disk
great red spot
Winter Solstice
20. A point in the sky where meteors appear to come from during a shower
Doppler Shift
Plague
radiant
MOONS: thickest atmosphere
21. A star that is in the process of forming. It glows from gravitational contraction
Precession
Umbra
MOONS: roundest shape
protostar
22. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
The Local Group
Apollo asteroids
great dark spots
Spectroscopy
23. How is the Hubble Law consistent with an expanding universe?
regolith
Electromagnetic Radiation: Radio
least dense
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.
24. The amount an image is enlarged by a telescope
zone
Magnification
Penumbra
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
25. The location in the Milky Way where stars orbit like a solid wheel
contrast northern lowlands and the southern highlands of mars...
Bulge
Lagrangian Razor
Density Wave
26. Any change in the speed or direction of an object's motion
acceleration
Sidereal Day
homogeneous
Cepheid Variable
27. 10^2 nm 10^7 nm
Atomic Number
regolith
Electromagnetic Radiation: Gamma Ray
Light Pollution
28. 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 ________.
Flat - Flat
Olber's paradox
HII Region
Dark Matter
29. The point in its orbit where a planet is nearest the sun
Most dense
differential rotation
meteorite
Perihelion
30. A continuous spectrum of light missing energy at a few wave lengths.
Light: travels like a wave - detected like a particle
Supernova (You can be my supernova girl)
Absorption Spectrum
Kuiper belt
31. The location around an atom where an electron resides.
Thermal Equilibrium
Energy Level
Annular Eclipse
Granules
32. 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
Wein's Law
Prominence
Cosmic Microwave Background (CMB)
33. The law that predicts the possible types of spectra.
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34. Saying that the sky should not get dark at night because all lines of sight end on a star meaning that the night sky should be ablaze BUT the big bang - because the universe had a beginning - says that the sky gets dark because out in space - galaxie
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35. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
superclusters
cosmology
Planck time
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
36. Jupiter
inferior planets
Disk
fastest rotation
Radio Galaxy
37. Form honeycomb like patterns surrounding empty or nearly empty voids.
planetary nebula
superclusters
Chandrasekhar Limit
Filament
38. Then the Sun moves from north to south across the celestial equator (about September 23)
Primary Mirror
OB Associations
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Autumnal Equinox
39. The law that syas light energy from a blackbody increases as (temperature^4)
Grand design spirals
Stephen-Boltzman Law
general star population
Jovian Planets
40. 1μm 100 nm
Absolute Magnitude
Electromagnetic Radiation: Visible Light
Planetary Nebula
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
41. The Big Bang says that the universe has not existed forever. It had a distinct beginning about 14 billion years ago called the 'Big Bang'. Therefore light from any object more than 14 billion light years away has not had time to reach us. The other p
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42. 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
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
Hubble law
Roundest orbit
Most dense
43. Centered on the Earth
differential rotation
Red Giant Branch Star
highlands
Geocentric
44. A change in the wavelength of light caused by a motion between the observer and light (or wave) source (blue shift if getting closer - red shift if moving away)
Coronal Loop
Spectroscopic Parallax
Doppler Shift
greatest elongation
45. The material from which the solar system formed
solar nebula
Celestial Equator
Rich Cluster
Population 1 vs Population 2 stars
46. Where is the center of the expansion
MOONS: largest size
Io (jupiters moon)
resonance
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.
47. A telescope that uses mirrors to focus light
Photon
Electromagnetic Radiation: Infrared
Ionization
Reflector
48. The measure of a variable star's apparent magnitude as it brightens and dims with time
Extrasolar Planet
Synchrotron Rotation
Light Curve
Radio Galaxy
49. The rate of expansion of the universe.
Prominence
Electromagnetic Radiation: Infrared
meteor
Hubble constant
50. The apparent path of the Sun through the stars on the celestial sphere.
Chromosphere
Hipparchus
Ecliptic
Trojan asteroids