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Test your basic knowledge |
Cosmology
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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. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
weight
planetary nebula
tectonics of Venus
blazar
2. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
isotropic
quasar
MOONS: larger than mercury
Ammonia - methane - and water
3. IO
Eyepiece Lens
MOONS: most geologically active
Kirkwood gaps
Population 1 vs Population 2 stars
4. The point in its orbit where a planet is farthest from the sun
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.
Superior planets
aphelion
dark energy
5. A large and bright but cool star.
regolith
superclusters
Planck time
Red Giant
6. A large and bright but cool star.
Disk
Energy Level
Red Giant
highlands
7. Venus (retrograde)
slowest rotation
Kuiper belt
bulge
Cassini division
8. When the Sun moves from south to north across the celestial equator (about March 21)
Kirkwood gaps
Vernal Equinox
Oort cloud
condensation temperature
9. The distance a moon can be from a planet before shattering from tidal forces
Granules
fusion crust
asteroid
roche limit
10. 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.
Geocentric
Kuiper belt
Cosmic Microwave Background (CMB)
Coronal Loop
11. The organization of clusters of galaxies into sheets and strings
planetary nebula
shape and color of SPIRAL galaxies
Rich Cluster
Supercluster
12. That which is responsible for Jupiter's magnetic field
Liquid metallic hydrogen
Secondary Mirror
Oort Cloud
Differential Rotation
13. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Turn off Point
Bok Globule
White Dwarf
If it is in a denser medium - such as glass - it will move slower
14. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Dark matter candidates
radiation pressure
Celestial Equator
Neutron Star
15. A rock or iron specimen that has fallen from space
MOONS: most geologically active
nucleus
meteorite
Summer Solstice
16. A telescope that uses mirrors to focus light
deferent
Flocculent spirals
Reflector
Chandrasekhar Limit
17. A younger cluster of stars - found in the galaxy disk
H-are Diagram
Electromagnetic Radiation: Ultraviolet Light
Open Cluster
Red Giant
18. A term referring to the orbital character of stars near the Sun
hottest surface
Differential Rotation
Milky way Galaxy
Hubble constant
19. Venus
hottest surface
Particle Horizon
Ammonia - methane - and water
Resolving Power
20. Mercury
least dense
Oort cloud
Pixel
thinnest atmosphere
21. 1 mm 1μm
terrestrial planet
solar nebula
Electromagnetic Radiation: Infrared
partile horizon
22. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
Limb darkening
opposition
Liquid metallic hydrogen
inferior planets
23. The sinking of denser elements to the center of a young molten planet
anorthosite
Metals
chemical differentiation
Spectroscopic parallax
24. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Eclipses of the Moons of Jupiter
Light: travels like a wave - detected like a particle
tectonics of Earth
Main Sequence
25. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Active Optics
Sidereal Day
Make up of the jovian planets
Seyfert galaxy
26. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
Penumbra
mapping the structure of Milky Way disk
density parameter
contrast northern lowlands and the southern highlands of mars...
27. Matter that reveals itself only through its gravitational attraction
Dark Matter
Disk
Summer Solstice
shape and color of ELLIPTICAL galaxies
28. The first rock-sized bodies that formed in the solar nebula from dust grains
chondrite
Cepheid variables
Kirchhoff's Law
Reflector
29. 10^2 nm 10^7 nm
Electromagnetic Radiation: Gamma Ray
Kuiper belt
Poor Cluster
Celestial Sphere
30. 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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31. A repeated - periodic push or pull capable of summing into a larger push or pull
resonance
plate tectonics
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Dwarf planets
32. Earth
Most dense
Active Optics
Black Hole
Chromosphere
33. A change in the appearance of the sun at the edge of the solar disk
AGN
Proton-proton chain
E=mc2
Limb darkening
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. Dark - reddish - low-pressure bands in Jupiter's atmosphere
Neutron Star
Colestial Pole
belt
Ammonia - methane - and water
36. An object that may remain after a star explodes
blazar
Enke gap
synchronous rotation
Neutron Star
37. Dark areas on the sun that are cooler than the surrounding photosphere
Shepherd satellite
Sunspots
Hubble constant
Convection
38. Jupiter
most moons
radiation pressure
Proton-proton chain
Callisto (Jupiter)
39. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
Halo
Thickest atmosphere
bulge
plate tectonics
40. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
Turn off Point
Kuiper belt
Dark Nebula
Europa (Jupiters moon)
41. A galaxy emitting large amounts of energy at long wavelengths.
radio galaxy
slowest rotation
Dark Nebula
retrograde motion
42. The high- temperatature outer layer of the sun
High Velocity Stars
Corona
Secondary Mirror
The Big Bang Theory
43. When massive objects bend space and time enough to create multiple images of an object located behind them
Astronomical Unit
Sunspot cycle
Umbra
Gravitational Lens
44. A word meaning 'the same in all directions.'
Open Cluster
Ionization
isotropic
blazar
45. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
Synodic Day
3 reasons we orbit satellites to observe universe
epicycle
Blackbody
46. Very center of galaxy. suggestion of a black hole
nucleus
Apparent Magnitude
inferior planets
bulge
47. When material is heated and moves taking the heat energy with it
High Velocity Stars
Convection
nova
Precession
48. Saturn
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.
Eclipses of the Moons of Jupiter
difference between maria and highlands of the moon.
least dense
49. A spread of light with an uninterrupted wavelength distribution of energy.
Light: travels like a wave - detected like a particle
Continuous Spectrum
Gamma-ray Burst
Gamma ray bursts
50. Half of the longest diameter across an ellipse
condensation temperature
semimajor axis
fastest rotation
Perihelion
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