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Test your basic knowledge |
Cosmology
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Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
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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 entity from which the whole universe is postulated to have come from.
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.
Bok Globule
cosmic singularity
blazar
2. The mix of pure photon energy that emerged at the start of the universe.
cosmic fireball
nova
direct motion
Differential Rotation
3. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
force
The Local Group
Continuous Spectrum
chemical differentiation
4. 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
Asymptotic giant Branch Star
accretion disk
standard candle
Emission Spectrum
5. When the Sun is farthest south of the celestial equator (About December 22)
contrast northern lowlands and the southern highlands of mars...
Winter Solstice
semimajor axis
Spectroscopic parallax
6. The particle horizon is the farthest we can see. It exists because the universe had a beginning and thus a definite age. Light from distances farther away from the particle horizon have not had time to reach us yet.
Thickest atmosphere
Particle Horizon
Nucleus
CMB
7. The displacement of spectral lines to redder colors caused by the expansion of the universe.
Hipparchus
cosmological red shift
Light-Year
Radio Galaxy
8. An element of a highly efficient - two-dimensional electronic light detector
differential rotation
Pixel
Cosmic Microwave Background
Asymptotic giant Branch Star
9. A huge sphere of tenuous gas surrounding the nucleus of a comet
coma
Hipparchus
Zenith
planetary nebula
10. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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11. A term referring to Earth-like planets
acceleration
terrestrial planet
mapping the structure of Milky Way disk
Light-Year
12. 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.
quarks
Celestial Equator
mass
tectonics of Venus
13. All possible types of energy that can be emitted and absorbed by atoms.
A family of radiant energy- includes light
High Velocity Stars
Electromagnetic Radiation
Olber's paradox
14. A small chunk of rock in space
solar nebula
Apparent Magnitude
roche limit
meteoriod
15. Small moons that maintain the shape of rings around Saturn and Uranus
Shepherd satellite
Energy Level
condensation temperature
Electromagnetic Radiation
16. The projection of the Earth's equator onto the celestial sphere.
Light Gathering Power
Celestial Equator
H2 Regions
Celestial Sphere
17. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Oort cloud
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
Spectroscopic Parallax
acceleration
18. Matter that reveals itself only through its gravitational attraction.
Synchrotron Rotation
asteroid
dark matter
Radio Galaxy
19. The location of a supermassive black hole
Nucleus
Doppler Shift
Refractor
Population 1 vs Population 2 stars
20. A star without enough mass to begin hydrogen fusion
Coronal Loop
meteoriod
superclusters
Brown dwarf
21. An entity that is likely in the nucleus of most - if not all - galaxies.
supermassive black hole
Dark Matter
bulge
chemical differentiation
22. A volume of space where few - if any - galaxies are located
evidence of water on mars
Void
great dark spots
Cepheid variables
23. A collection of galaxies like the one the Milky Way belongs to
Focal Length
homogeneous
chemical differentiation
Poor Cluster
24. 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
Spectroscopic parallax
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.
Total Eclipse
25. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Ionization
cosmic fireball
The Local Group
Light Curve
26. The law that predicts the possible types of spectra.
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27. Extends to a distance of 50000AU. Same objects as in the Kuiper belt-when they fall in toward the sun they become comets. Debris from comets hitting the Earths atmosphere cause meteor showers.
Absolute Magnitude
neutrino
Oort Cloud
Prominence
28. Dark areas on the sun that are cooler than the surrounding photosphere
Color Index
Parallax
Sunspots
standard candle
29. What Ole Roemer used to measure the speed of light in a vacuum
Sunspots
Open Cluster
Thermonuclear Fusion
Eclipses of the Moons of Jupiter
30. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Sb spiral galaxy
Make up of the terrestrial planets
Asymptotic giant Branch Star
Gravitational Lens
31. The point in its orbit where a planet is farthest from the sun
Titus-Bode Law
Coronal Loop
aphelion
Electromagnetic Radiation: Ultraviolet Light
32. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
inferior planets
Kuiper belt
Apollo asteroids
Colestial Pole
33. A perfect absorber and radiator of electromagnetic radiation.
radio galaxy
Synchrotron Rotation
Electromagnetic Radiation: Radio
Blackbody
34. Moon in less than the angular diameter of the Sun.
Disk
Kuiper belt
Annular Eclipse
Cassegrain Focus
35. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
Cosmic Microwave Background (CMB)
shape and color of SPIRAL galaxies
supernova
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.
36. A high-pressure bulge in Neptune's southern hemisphere
Occam's razor
acceleration
Prominence
great dark spots
37. 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.
era of recombination
Trojan asteroids
contrast northern lowlands and the southern highlands of mars...
Nova
38. An element of a highly efficient - two-dimensional electronic light detector
Population 1 vs Population 2 stars
Pixel
tectonics of Venus
terrestrial planet
39. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
jovian
Self-Propogating Star Formation
Kirkwood gaps
bulge
40. 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)
Particle Horizon
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.
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
quasar
41. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Light Gathering Power
Halo
Negative - Diverge - Less than 1
Jovian Planets
42. The oldest grouping of stars - found in the galaxy halo
Pixel
Big Bang
Globular Cluster
Kirchhoff's Law
43. 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 _____.
Flat - Remain Parallel - Exactly 1
Synodic Day
coma
Supernova (You can be my supernova girl)
44. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Penumbra
Blackbody Curve
fewest moons
Sc spiral galaxy
45. VENUS
Focal Plane
Pulsar
Neutron Star
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
46. Earth
H2 Regions
Most dense
opposition
E=mc2
47. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
cosmological red shift
Dark Nebula
Quasar
Precession
48. The 'edge' of the universe. Light beyond this has not reached us yet.
partile horizon
Gamma ray bursts
Oort Cloud
comet
49. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Wein's Law
Sb spiral galaxy
quasar
tectonics of Mars
50. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
widmanstatten pattern
Black Hole
Continuous Spectrum
Absorption Spectrum
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