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Test your basic knowledge |
Cosmology
Start Test
Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
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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. Any class of objects with a uniform luminosity used to determine distance.
Cosmic Microwave Background (CMB)
Largest diameter
Winter Solstice
standard candle
2. A star that has become a red giant for the second and final time. It is burning helium to carbon in a shell surrounding the core
difference between maria and highlands of the moon.
Asymptotic giant Branch Star
cosmological principle
great dark spots
3. An element of a highly efficient - two-dimensional electronic light detector
Density Wave
density
Plague
Pixel
4. A galaxy sending out a stream of material from its nucleus
Energy Level
dark matter
Radio Galaxy
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.
5. The mirror that determines the focus configuration of a reflector
Secondary Mirror
Planetary Nebula
standard candle
fastest rotation
6. Infinitely long -> 10 cm
Limb darkening
fusion crust
Electromagnetic Radiation: Radio
If it is in a denser medium - such as glass - it will move slower
7. A bright area of higher temperature that often proceeds the formation of sunspots.
Plague
dark energy
regolith
Electromagnetic Radiation
8. Theory virtually demands that the geometry of the universe be ______. Results of measuring lumps in the cosmic background radiation indicate that the universe geometry is ________.
plate tectonics
Flat - Flat
Ground State
Summer Solstice
9. The source of the force that is accelerating the expansion rate of the universe.
Electron
dark energy
Electromagnetic Radiation: X-Ray
fastest rotation
10. The lens that gathers the light in a refractor
cosmic fireball
radiation pressure
Objective Lens
Black Hole
11. The rate of expansion of the universe.
Color Index
Roundest orbit
difference between maria and highlands of the moon.
Hubble constant
12. Material that shoots rapidly out into space. Flares cause Auroras
Oort cloud
Kirkwood gaps
Flare
Jovian Planets
13. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
Radiative Diffusion
Total Eclipse
mass
Cosmic Microwave Background (CMB)
14. The law that syas light energy from a blackbody increases as (temperature^4)
Sa spiral galaxy
Winter Solstice
Stephen-Boltzman Law
Planck time
15. The measure of a variable star's apparent magnitude as it brightens and dims with time
Interstellar Extinction
Titus-Bode Law
Light Curve
The Big Bang Theory resolves Olber's Paradox
16. When a planet lines up with the sun inthe sky
conjunction
Flare
Chandrasekhar Limit
MOONS: larger than mercury
17. What is the universe expanding into?
CMB
Most dense
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.
Olber's paradox
18. A star that is in the process of forming. It glows from gravitational contraction
SETI
protostar
Red Giant
matter dominated universe
19. Long - meandering cliff formed when a planet surface cools and shrinks
accretion
radiation pressure
scarp
fewest moons
20. The family of radiant energy that includes light as a subset
Electromagnetic Radiation: Radio
Electromagnetic Radiation
matter dominated universe
Objective Lens
21. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Nebula
Kuiper belt
great dark spots
greatest elongation
22. A two-filter measure of the color - and hence temperature - of a star.
Color Index
Primary Mirror
Electromagnetic Radiation: Microwave
Proton-proton chain
23. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Halo
Dark Nebula
Kuiper belt
shape and color of SPIRAL galaxies
24. Venus
Apparent Magnitude
Thickest atmosphere
chondrite
Largest diameter
25. A repeated - periodic push or pull capable of summing into a larger push or pull
resonance
Oort cloud
synchrotron radiation
density waves
26. An empirical scheme for predictin ghe orbital distances of planets
Largest diameter
CNO Cycle
planetary nebula
Titus-Bode Law
27. A fusion process in which protons build together to form helium
Light Curve
Olber's paradox
Photometry
Proton-proton chain
28. A galaxy emitting large amounts of energy at long wavelengths.
Nova
radio galaxy
Self-Propogating Star Formation
Supercluster
29. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
force
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
rotation curve=winding dilemma?
tectonics of Venus
30. The Greek philosopher responsible for making the stellar magnitude scale.
Titus-Bode Law
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.
Hipparchus
Galilean satellite
31. In what chemical form are jupiters nitrogen - carbon and oxygen?
Spectroscopic Parallax
Celestial Equator
Ammonia - methane - and water
fusion crust
32. A high-pressure bulge in Neptune's southern hemisphere
Maria
condensation temperature
great dark spots
Cosmic Microwave Background (CMB)
33. A small and dim but hot star.
White Dwarf
Inverse Square Law
fastest rotation
great dark spots
34. Why do Galaxies move very rapidly in the interiors of the dense clusters?
molecular clouds
Io (jupiters moon)
Population 1 vs Population 2 stars
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
35. The era when the ratio of matter to energy greatly favored matter. (verses radiation dominated universe where it was opaque. Matter is now dominated by gravity not photons)
matter dominated universe
Filament
hottest surface
Granules
36. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Sunspots
Bulge
Light Gathering Power
Negative - Diverge - Less than 1
37. The point in its orbit where a planet is farthest from the sun
aphelion
Sa spiral galaxy
great red spot
CCD
38. A bright area of higher temperature that often proceeds the formation of sunspots.
Molecular Clouds
Planck time
least dense
Plague
39. A plot of star absolute magnitude verses spectral type.
Cepheid variables
Interstellar Extinction
H-are Diagram
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
40. 1 mm 1μm
thinnest atmosphere
Black Hole
Stephen-Boltzman Law
Electromagnetic Radiation: Infrared
41. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
Kirkwood gaps
supermassive black hole
Active Optics
shape and color of SPIRAL galaxies
42. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Synodic Day
Void
Disk
Dark matter candidates
43. The high- temperatature outer layer of the sun
hottest surface
Seeing
MOONS: larger than mercury
Corona
44. A galaxy sending out a stream of material from its nucleus
Kirchhoff's Law
Electromagnetic Radiation
Parsec
Radio Galaxy
45. Jupiter - Saturn - Uranus - Neptune
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
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Asymptotic giant Branch Star
Jovian Planets
46. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
Chromosphere
Secondary Mirror
Gamma ray bursts
quarks
47. 10 cm -> 1 mm
Callisto (Jupiter)
Absolute Magnitude
Focal Plane
Electromagnetic Radiation: Microwave
48. A measure of the ability of a telescope to see fine detail
Flare
Resolving Power
Stephen-Boltzman Law
Sb spiral galaxy
49. The light produced when particles from the sun collide with atmospheric molecules
Absolute Magnitude
aurora
Rich Cluster
comet
50. A star fusing hydrogen to helium in it's core
fusion crust
Main Sequence Stars
Quasar
differential rotation
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