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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-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
tectonics of Venus
Electromagnetic Radiation
Olber's paradox
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
2. Jupiter
High Velocity Stars
most moons
roche limit
Cosmic Microwave Background
3. Matter so dense that even light cannot escape its gravity
Heliocentric
Black Hole
Thermal Equilibrium
Electromagnetic Radiation: Ultraviolet Light
4. Half of the longest diameter across an ellipse
direct motion
weight
semimajor axis
Kirchhoff's Law
5. The seasonal shifting of a nearby star's position relative to more distant objects.
regolith
Parallax
Absorption Spectrum
Radio Galaxy
6. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
Triple Alpha rocess
Make up of the terrestrial planets
Gamma ray bursts
Rich Cluster
7. The rock that makes up the lunar highlands
Summer Solstice
solar nebula
Photosphere
anorthosite
8. A small spherical dark nebula
Meridian
Bok Globule
Geocentric
Thermonuclear Fusion
9. Large nebula consisting of very cold gas and dust
chondrite
evidence of water on mars
Molecular Clouds
roche limit
10. The rotation period of the Earth measured relative to the stars.
great dark spots
Sidereal Day
Light Gathering Power
retrograde motion
11. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
Photosphere
cosmic singularity
neutrino
comet
12. A galaxy emitting large amounts of energy at long wavelengths.
Nova
radio galaxy
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
Roundest orbit
13. The amount an image is enlarged by a telescope
MOONS: larger than mercury
Granules
Limb darkening
Magnification
14. The larger bodies that formed early in teh solar nebula that were chemically differentiated
Annular Eclipse
planetesimal
Light-Year
Blackbody Curve
15. The material from which the solar system formed
Bulge
Supercluster
Electromagnetic Radiation
solar nebula
16. Hot cells of gas that rise and fall in the hotosphere
Granules
Ecliptic
Self-Propogating Star Formation
Roundest orbit
17. The Big Bang was not an explosion of matter into empty space - like the explosion of a bomb. Instead - it was an emergence of space and time filled with pure energy where before none of this was present. The point from which is emerged is called the
Planetary Nebula
The Big Bang Theory
Bok Globule
isotropic
18. A star fusing hydrogen to helium in it's core
comet
Main Sequence Stars
Hydrostatic Equilibrium
Electromagnetic Radiation: Infrared
19. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Make up of the jovian planets
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
Thermal Equilibrium
Globular Cluster
20. A distance measure determined by the shifting of a star against the background sky every 6 months.
Cosmological Principle
Hubble constant
zone
Parsec
21. 10 nm 10^2 nm
Electromagnetic Radiation: X-Ray
Halo
H-are Diagram
Parallax
22. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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23. Saturn
A family of radiant energy- includes light
Main Sequence
least dense
weight
24. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
Thermal Equilibrium
cosmological principle
Instability strip
HII Region
25. 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.
Oort cloud
open star clusters
acceleration
Ole Roemer
26. A younger cluster of stars - found in the galaxy disk
Cosmological Principle
cosmology
How is winding dilemma solved?
Open Cluster
27. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
Gamma ray bursts
homogeneous
most moons
Hydrostatic Equilibrium
28. Long - meandering cliff formed when a planet surface cools and shrinks
300000 KM/sec
Emission Spectrum
scarp
radio galaxy
29. Jupiter
great red spot
Largest diameter
Maria
Poor Cluster
30. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Halo
critical density
Photosphere
Ammonia - methane - and water
31. A bridge of material held in position above the solar surface. They can remain for hours even days
Absorption Spectrum
Prominence
CCD
Precession
32. The lowest energy of an atom.
contrast northern lowlands and the southern highlands of mars...
Ground State
dark energy
Interstellar Extinction
33. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
radiation dominated universe
Population 1 vs Population 2 stars
Nova
The Big Bang Theory
34. Earth
Hubble law
Most dense
H-are Diagram
Cosmic Microwave Background
35. Sc galaxies
Limb darkening
open star clusters
greatest elongation
Flocculent spirals
36. Form honeycomb like patterns surrounding empty or nearly empty voids.
Total Eclipse
Thermal Equilibrium
Differential Rotation
superclusters
37. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Eclipses of the Moons of Jupiter
Roundest orbit
plate tectonics
Active Optics
38. A long-lived high-pressure bulge in Jupiter's southern hemisphere
Light Pollution
CMB
great red spot
belt
39. A star that erratically and explosively brightens and dims
Jovian Planets
A family of radiant energy- includes light
Nova
Focal Length
40. A word used in astronomy to describe all elements besides hydrogen and helium
Metals
Hubble constant
interstellar dust
Halo
41. Dark areas on the sun that are cooler than the surrounding photosphere
era of recombination
Supernova (You can be my supernova girl)
Sunspots
Cassegrain Focus
42. Hydrogen and helium (mainly)
Make up of the jovian planets
Brown dwarf
hottest surface
tectonics of Earth
43. A representation of the changes in color and brightness of an evolving protostar.
Radio Galaxy
Cepheid Variable
Hyashi track
Oort Cloud
44. A huge sphere of tenuous gas surrounding the nucleus of a comet
density parameter
Ganymede (Jupiter)
coma
terrestrial planet
45. The part of the Milky way that has on-going star formation
Disk
tectonics of Mars
synchronous rotation
Sa spiral galaxy
46. The high- temperatature outer layer of the sun
Seyfert galaxy
Corona
quasar
Self-Propogating Star Formation
47. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
Plague
blazar
comet
radio galaxy
48. Approximate speed of light in a vacuum
Largest diameter
roche limit
Hubble constant
300000 KM/sec
49. Flat disk with gas - dust - H2 regions - molecular clouds - dust young stars and remnants of old planetary nebula and supernova remnants. stars spin together with similar velocities called differential rotation
disk
supernova
Light: travels like a wave - detected like a particle
Sunspots
50. The apparent path of the Sun through the stars on the celestial sphere.
Ecliptic
Chromosphere
Thermonuclear Fusion
planetary nebula