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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. The amount an image is enlarged by a telescope
Spectral Lines
Triple Alpha rocess
Shepherd satellite
Magnification
2. The powdered stone fragments that make up the lunar 'soil'
Drake equation
contrast northern lowlands and the southern highlands of mars...
regolith
most moons
3. The entity responsible for spiral arms in grand-design spiral galaxies
Light Gathering Power
Density Wave
White Dwarf
Cassini division
4. The process that powers the sun and hydrogen bombs
Oort Cloud
Electromagnetic Radiation: Visible Light
coma
Thermonuclear Fusion
5. The study of the universe as a whole.
retrograde motion
Halo
Black Hole
cosmology
6. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
homogeneous
HII Region
regolith
If it is in a denser medium - such as glass - it will move slower
7. Any class of objects with a uniform luminosity used to determine distance.
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.
meteor
standard candle
Dark matter candidates
8. The equation that describes how matter equates with energy
radio lobe
E=mc2
If it is in a denser medium - such as glass - it will move slower
Limb darkening
9. The law stating that hotter blackbodies look bluer than cooler blackbodies.
10. A measure of the force of gravity on an object
self-propagating star formation
weight
chemical differentiation
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.
11. 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.
Main Sequence
CMB
Gamma ray bursts
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
12. A high-pressure bulge in Neptune's southern hemisphere
Spectroscopy
H2 Regions
great dark spots
MOONS: roundest shape
13. Moon in less than the angular diameter of the Sun.
300000 KM/sec
Annular Eclipse
zone
open star clusters
14. 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
15. A bright area of higher temperature that often proceeds the formation of sunspots.
radiation dominated universe
Plague
density waves
open star clusters
16. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Pixel
Electromagnetic Radiation: Ultraviolet Light
quasar
E=mc2
17. An energetic event taking place in the early universe
Inverse Square Law
Black Hole
belt
Gamma-ray Burst
18. 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.
Astronomical Unit
Autumnal Equinox
Kirchhoff's Law
Jupiters red spot
19. A change in the appearance of the sun at the edge of the solar disk
Turn off Point
Refractor
Supernova (You can be my supernova girl)
Limb darkening
20. The location in the Milky Way where stars orbit like a solid wheel
Oort cloud
least dense
Bulge
neutrino
21. A spinning neutron star
Spectral Lines
Pulsar
resonance
Nucleus
22. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
great dark spots
zone
CCD
Gamma ray bursts
23. The powdered stone fragments that make up the lunar 'soil'
Total Eclipse
Parsec
Light Gathering Power
regolith
24. The 'edge' of the universe. Light beyond this has not reached us yet.
Secondary Mirror
zone
Liquid metallic hydrogen
partile horizon
25. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Absorption Spectrum
Quasar
dark energy
Void
26. What are the three possible geometries of the universe?
great red spot
Open - flat - and closed.
Electromagnetic Radiation: Infrared
MOONS: larger than mercury
27. A planet orbiting about a distant star
Cosmic Microwave Background
Largest diameter
Extrasolar Planet
Enke gap
28. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
Seyfert galaxy
HII Region
mass
Umbra
29. Any class of objects with a uniform luminosity used to determine distance.
Lagrangian Razor
standard candle
MOONS: largest size
Granules
30. A faint - remarkably uniform distribution of radiation in space
Cosmic Microwave Background
Coldest surface
Photometry
planetesimal
31. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Secondary Mirror
Sc spiral galaxy
dark matter
Galilean satellite
32. A long-lived high-pressure bulge in Jupiter's southern hemisphere
Atomic Number
highlands
reflection star clusters
great red spot
33. 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
34. The law that describes the blackbody curve - and let to quantum mechanics.
35. Venus
Liquid metallic hydrogen
Roundest orbit
Triple Alpha rocess
accretion disk
36. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Interstellar Extinction
tectonics of Earth
MOONS: larger than mercury
Photosphere
37. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Kirkwood gaps
most moons
isotropic
Ole Roemer
38. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Active Optics
Open - flat - and closed.
CNO Cycle
accretion
39. A small chunk of rock in space
Turn off Point
Pixel
isotropic
meteoriod
40. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
resonance
cosmic singularity
Electromagnetic Radiation: Visible Light
opposition
41. A term referring to the orbital character of stars near the Sun
Ole Roemer
Colestial Pole
Differential Rotation
Cosmological Principle
42. Long - meandering cliff formed when a planet surface cools and shrinks
scarp
Photosphere
tectonics of Venus
E=mc2
43. The shadow behind the Earth or Moon where the Sun is partially obscured.
aphelion
The Big Bang Theory resolves Olber's Paradox
Penumbra
mass
44. A crystalline patter found in iron meteorites
Cosmic Microwave Background
Hydrostatic Equilibrium
widmanstatten pattern
Europa (Jupiters moon)
45. The cosmological principle is the assumption that the universe is isotropic and homogeneous.The Big Bang assumes it to be a correct principle so that what we observe is exactly like What is too far away to be observed.
Refractor
Cosmological Principle
roche limit
Dark Nebula
46. The rotation of a star or planet at different speeds at its equator and poles
roche limit
Oort cloud
Oort Cloud
differential rotation
47. A word meaning 'the same everywhere throughout.'
Umbra
slowest rotation
cosmic singularity
homogeneous
48. Neptune or uranus
Coldest surface
isotropic
great red spot
contrast northern lowlands and the southern highlands of mars...
49. That which is responsible for Jupiter's magnetic field
open star clusters
nucleus
Liquid metallic hydrogen
planetary nebula
50. A distance measure determined by the shifting of a star against the background sky every 6 months.
cosmological principle
Parsec
standard candle
Kirchhoff's Law