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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. When material is heated and moves taking the heat energy with it
Eclipses of the Moons of Jupiter
aphelion
Convection
chemical differentiation
2. What is the universe expanding into?
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
Red Giant
Secondary Mirror
3. 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.
scarp
Jupiters red spot
Sc spiral galaxy
Sc spiral galaxy
4. Young clusters in disk are irregularly shaped since they have no time to relax into the rounder relaxed shape of globular clusters-will constantly be torn apart and assimilated.
Halo
Asymptotic giant Branch Star
open star clusters
resonance
5. Material that shoots rapidly out into space. Flares cause Auroras
chemical differentiation
The Big Bang Theory resolves Olber's Paradox
Flare
Trojan asteroids
6. A younger cluster of stars - found in the galaxy disk
cosmology
MOONS: most geologically active
Open Cluster
Light: travels like a wave - detected like a particle
7. Earth
Heliocentric
Most dense
Grand design spirals
Neutron Star
8. A small and dim but hot star.
Resolving Power
tectonics of Earth
White Dwarf
Kuiper belt
9. 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.
quarks
conjunction
Electromagnetic Radiation: Infrared
era of recombination
10. Collections of young - hot stars
dark matter
Main Sequence
OB Associations
Corona
11. A spectrum of light with energy at only a few wavelengths.
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
300000 KM/sec
Emission Spectrum
Seeing
12. Large nebula consisting of very cold gas and dust
Color Index
Molecular Clouds
Oort cloud
Pulsar
13. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
Asymptotic giant Branch Star
Titus-Bode Law
Sunspot cycle
self-propagating star formation
14. The mix of pure photon energy that emerged at the start of the universe.
cosmic fireball
Pulsar
Supercluster
Liquid metallic hydrogen
15. Material that shoots rapidly out into space. Flares cause Auroras
Supercluster
Flare
weight
Proton-proton chain
16. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Electromagnetic Radiation
Nebula
planetesimal
Gamma-ray Burst
17. The slow wobble of the Earth on its rotation axis.
Particle Horizon
Precession
H-are Diagram
Photon
18. Either Io -Europa - Ganymede - or Callisto
reflection star clusters
Photometry
Galilean satellite
Bulge
19. A measure of the force of gravity on an object
belt
fewest moons
Thickest atmosphere
weight
20. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
CCD
Radio Galaxy
hottest surface
Molecular Clouds
21. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
smallest diameter
asteroid
CCD
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
22. The high- temperatature outer layer of the sun
radio galaxy
Corona
semimajor axis
Absorption Spectrum
23. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Oort cloud
Kirchhoff's Law
MOONS: thickest atmosphere
Sc spiral galaxy
24. Distance from sun to nucleus- 8 kiloparsecs (26000 LY) - diameter of Milky way- 150000 LY - length for sun to orbit once around milky way- 250 million years
Milky way Galaxy
Hipparchus
Interstellar Extinction
Photosphere
25. The temp at which a substance in the vacuum of space solidifies
terrestrial planet
Electromagnetic Radiation: Ultraviolet Light
Apparent Magnitude
condensation temperature
26. The law that describes the blackbody curve - and let to quantum mechanics.
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27. A galaxy emitting large amounts of energy at long wavelengths.
Particle Horizon
Supercluster
radio galaxy
great red spot
28. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
matter dominated universe
Colestial Pole
Make up of the terrestrial planets
Sb spiral galaxy
29. The normal eastward movement of a planet against the background of hte distant stars.
Flat - Flat
direct motion
MOONS: most geologically active
evidence of water on mars
30. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Kirkwood gaps
Sc spiral galaxy
Flat - Flat
Rich Cluster
31. The larger bodies that formed early in teh solar nebula that were chemically differentiated
planetesimal
Chandrasekhar Limit
Stephen-Boltzman Law
Maria
32. 1 mm 1μm
Vernal Equinox
Dark matter candidates
Electromagnetic Radiation
Electromagnetic Radiation: Infrared
33. 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
Flat - Flat
mare basalt
Apollo asteroids
34. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Halo
asteroid
Plank's Law
great red spot
35. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Dark Nebula
partile horizon
Triple Alpha rocess
acceleration
36. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
molecular clouds
MOONS: roundest shape
Horizontal Branch Star
Proton-proton chain
37. A location on an H-are Diagram where evolving stars pulsate
White Dwarf
Emission Spectrum
Instability strip
cosmology
38. A faint - remarkably uniform distribution of radiation in space
White Dwarf
Cosmic Microwave Background
Dark Matter
Maria
39. The most mass a white dwarf can have before collapsing to a neutron star
Titus-Bode Law
Chandrasekhar Limit
shape and color of ELLIPTICAL galaxies
highlands
40. The surface of the sun
belt
Photosphere
Flocculent spirals
Nebula
41. First accurately measured the speed of light in a vacuum
quasar
Secondary Mirror
Ole Roemer
neutrino
42. Dark areas on the sun that are cooler than the surrounding photosphere
Hubble constant
evidence of water on mars
planetesimal
Sunspots
43. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Gravitational Lens
Oort Cloud
Callisto (Jupiter)
Refractor
44. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
Positive - Converge - Greater than 1
planetary nebula
radiation pressure
partile horizon
45. Form honeycomb like patterns surrounding empty or nearly empty voids.
evidence of water on mars
Extrasolar Planet
superclusters
Secondary Mirror
46. The apparent backward motion of a planet against the background of stars.
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
retrograde motion
meteor
Pixel
47. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Absolute Magnitude
rotation curve = dark matter?
Hyashi track
meteoriod
48. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
Planetary Nebula
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.
contrast northern lowlands and the southern highlands of mars...
radio galaxy
49. The fusion process that turns three helium nuclei into a carbon nucleus
Parallax
Triple Alpha rocess
Cepheid variables
Flocculent spirals
50. A word meaning 'the same in all directions.'
Parallax
Ecliptic
isotropic
Molecular Clouds