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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. Light-colored high-pressure bands in Jupiter's atmosphere
zone
Spectroscopic Parallax
Superior planets
terrestrial planet
2. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
Pulsar
Celestial Equator
epicycle
mare basalt
3. Orbit in Jupiters orbit
least dense
rotation curve = dark matter?
Ammonia - methane - and water
Trojan asteroids
4. What is the universe expanding into?
self-propagating star formation
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.
Thickest atmosphere
synchrotron radiation
5. The distance light travels in one year (=9.46x10^12km).
How is winding dilemma solved?
Apollo asteroids
Light-Year
Grand design spirals
6. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Resolving Power
Supernova (You can be my supernova girl)
Absolute Magnitude
OB Associations
7. Light scattered through the atmosphere that degrades astronomical images
molecular clouds
Asymptotic giant Branch Star
Light Pollution
superclusters
8. Mercury
thinnest atmosphere
Oort cloud
Black Hole
Hubble law
9. A streak of light in the atmosphere
Hydrostatic Equilibrium
meteor
comet
Geocentric
10. When one side of a body always faces the planet it revolves around
Bok Globule
Absorption Spectrum
synchronous rotation
shape and color of ELLIPTICAL galaxies
11. 1 mm 1μm
Electromagnetic Radiation: Infrared
Limb darkening
Electromagnetic Radiation: Microwave
Self-Propogating Star Formation
12. An entity that is likely in the nucleus of most - if not all - galaxies.
supermassive black hole
neutrino
Hipparchus
Atomic Number
13. A logarithmically scaled value for the measured brightness of a star.
Apparent Magnitude
radio galaxy
Vernal Equinox
semimajor axis
14. 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.
Occam's razor
Oort Cloud
Electromagnetic Radiation: Radio
CMB
15. A measure of the ability of a telescope to see fine detail
Resolving Power
deferent
We don't know. It might be but does not have to be.
Light Curve
16. Jupiter
Blackbody Curve
Brown dwarf
terrestrial planet
Largest diameter
17. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
Ammonia - methane - and water
density parameter
Heliocentric
protostar
18. Is space infinitely large?
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19. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
radio galaxy
Parallax
Ganymede (Jupiter)
Light: travels like a wave - detected like a particle
20. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Poor Cluster
Proton-proton chain
Electromagnetic Radiation: Visible Light
Neutron Star
21. The rate of expansion of the universe.
mapping the structure of Milky Way disk
Plank's Law
Hubble constant
Roundest orbit
22. The normal eastward movement of a planet against the background of hte distant stars.
direct motion
CCD
Astronomical Unit
Sb spiral galaxy
23. The displacement of spectral lines to redder colors caused by the expansion of the universe.
Limb darkening
cosmological red shift
Sunspot cycle
High Velocity Stars
24. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Light Gathering Power
Photosphere
Kirkwood gaps
Cassegrain Focus
25. 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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26. Poitns of gravitational stability in the orbit of a planet
Steady State Theory (Leads to Olber's Paradox)
Lagrangian Razor
Most dense
Emission Spectrum
27. Very center of galaxy. suggestion of a black hole
tectonics of Mars
Parallax
nucleus
scarp
28. A spectrum of light with energy at only a few wavelengths.
Quasar
Emission Spectrum
Meridian
bulge
29. The powdered stone fragments that make up the lunar 'soil'
Superior planets
Sb spiral galaxy
If it is in a denser medium - such as glass - it will move slower
regolith
30. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
Halo
Yes - frozen at the poles- remains protected from the suns rays
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.
evidence of water on mars
31. 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 _____.
terrestrial planet
Flat - Remain Parallel - Exactly 1
Supercluster
Continuous Spectrum
32. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
3 reasons we orbit satellites to observe universe
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
shape and color of ELLIPTICAL galaxies
acceleration
33. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Light Pollution
Occam's razor
difference between maria and highlands of the moon.
The Local Group
34. What causes the zones and belts on jupiter and saturn?
slowest rotation
cosmology
density parameter
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
35. The surface of the sun
Photosphere
E=mc2
most eccentric orbit
Poor Cluster
36. Why does the earth have few craters while the moon has many?
partile horizon
synchrotron radiation
Precession
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
37. An evolved star - past the helium flash that is burning helium to carbon in it's cores
Horizontal Branch Star
conjunction
Terrestrial Planets
Parsec
38. Titan
epicycle
MOONS: thickest atmosphere
cosmic fireball
meteorite
39. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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40. 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.
meteorite
aphelion
Electromagnetic Radiation
era of recombination
41. A galaxy sending out a stream of material from its nucleus
synchronous rotation
Callisto (Jupiter)
Globular Cluster
Radio Galaxy
42. The gap inthe outer portion of Saturn's A ring
Enke gap
Callisto (Jupiter)
chemical differentiation
We don't know. It might be but does not have to be.
43. Matter that reveals itself only through its gravitational attraction.
Plague
fewest moons
synchrotron radiation
dark matter
44. 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)
Doppler Shift
great red spot
dark matter
quasar
45. Large nebula consisting of very cold gas and dust
radiation dominated universe
E=mc2
Molecular Clouds
Gamma-ray Burst
46. Is space infinitely large?
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47. Venus
general star population
tectonics of Earth
Inverse Square Law
Roundest orbit
48. When massive objects bend space and time enough to create multiple images of an object located behind them
Liquid metallic hydrogen
Gravitational Lens
blazar
White Dwarf
49. A two-filter measure of the color - and hence temperature - of a star.
Cassegrain Focus
Color Index
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.
shape and color of SPIRAL galaxies
50. All wavelengths of light emitted by a blackbody.
differential rotation
Blackbody Curve
Umbra
Ammonia - methane - and water
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