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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. An object that may remain after a star explodes
Neutron Star
greatest elongation
Chandrasekhar Limit
neutrino
2. 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
Light-Year
dark matter
Extrasolar Planet
3. A star fusing hydrogen to helium in it's core
Main Sequence Stars
Granules
fastest rotation
Active Optics
4. When the Sun is farthest north of the celestial equator (about June 22)
Roundest orbit
MOONS: roundest shape
Cosmological Principle
Summer Solstice
5. When massive objects bend space and time enough to create multiple images of an object located behind them
most eccentric orbit
Absolute Magnitude
Gravitational Lens
Hydrostatic Equilibrium
6. The apparent backward motion of a planet against the background of stars.
Population 1 vs Population 2 stars
conjunction
The Local Group
retrograde motion
7. A high-pressure bulge in Neptune's southern hemisphere
Kirkwood gaps
molecular clouds
great dark spots
Enke gap
8. A star that is in the process of forming. It glows from gravitational contraction
open star clusters
Turn off Point
protostar
Radiative Diffusion
9. A perfect absorber and radiator of electromagnetic radiation.
Sidereal Day
Blackbody
Big Bang
Black Hole
10. Is there water on the moon?
Yes - frozen at the poles- remains protected from the suns rays
molecular clouds
Liquid metallic hydrogen
Poor Cluster
11. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Oort cloud
If it is in a denser medium - such as glass - it will move slower
Spectroscopic Parallax
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
12. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Sc spiral galaxy
deferent
Active Optics
Apollo asteroids
13. The sinking of denser elements to the center of a young molten planet
Interstellar Extinction
Cosmic Microwave Background (CMB)
chemical differentiation
tectonics of Earth
14. An entity that is likely in the nucleus of most - if not all - galaxies.
Poor Cluster
supermassive black hole
Sunspots
Seyfert galaxy
15. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
epicycle
matter dominated universe
Coronal Loop
dark energy
16. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
cosmic singularity
molecular clouds
Big Crunch
Jupiters red spot
17. Mercury and venus
AGN
fusion crust
fewest moons
smallest diameter
18. The temp at which a substance in the vacuum of space solidifies
Cassini division
condensation temperature
slowest rotation
Light Curve
19. A word used in astronomy to describe all elements besides hydrogen and helium
Hipparchus
Metals
H-are Diagram
Sb spiral galaxy
20. Venus (retrograde)
slowest rotation
Photometry
belt
Wein's Law
21. N=are*Fp(Ne)(Fl)(Fi)(Fc)(L) N: number of civilizations possible to communicate with are*: rate solar-like stars are created Fp: fraction of stars with planets Ne: number of planets like ours Fl: fraction of planets with life Fi: intelligent life Fc:
critical density
Vernal Equinox
Total Eclipse
Drake equation
22. The lens in a telescope used to determine the magnification
regolith
Eyepiece Lens
roche limit
self-propagating star formation
23. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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24. Collections of young - hot stars
Inverse Square Law
Hubble constant
Blackbody
OB Associations
25. Why does the earth have few craters while the moon has many?
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Electron
Self-Propogating Star Formation
planetesimal
26. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
tectonics of Earth
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
Heliocentric
quasar
27. A quantity measuring the stability of the Earth's atmosphere
superclusters
Seeing
Jovian Planets
synchrotron radiation
28. The process responsible for creating the arms of flocculent spiral galaxies
Self-Propogating Star Formation
Black Hole
Trojan asteroids
Big Bang
29. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Quasar
Bulge
Summer Solstice
Gravitational Lens
30. Electromagnetic Radiation
Focal Length
A family of radiant energy- includes light
opposition
Energy Level
31. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
Photosphere
Kirkwood gaps
Spectral Lines
tectonics of Mars
32. 10 nm 10^2 nm
epicycle
Light: travels like a wave - detected like a particle
Electromagnetic Radiation: X-Ray
A family of radiant energy- includes light
33. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Spectroscopic Parallax
Active Optics
Negative - Diverge - Less than 1
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
34. The fusion process that turns three helium nuclei into a carbon nucleus
Rich Cluster
Prominence
Steady State Theory (Leads to Olber's Paradox)
Triple Alpha rocess
35. 1-orbit aroudn the sun 2- are in hydrostatic equilibrium and 'mostly round' 3- have not cleared debris around its orbit 4- are not satellites
Io (jupiters moon)
Dwarf planets
quasar
most eccentric orbit
36. The displacement of spectral lines to redder colors caused by the expansion of the universe.
differential rotation
Maria
Pixel
cosmological red shift
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.
The Local Group
era of recombination
Most dense
Sa spiral galaxy
38. IO
MOONS: most geologically active
A family of radiant energy- includes light
MOONS: roundest shape
Electromagnetic Radiation: Radio
39. When a planet lines up with the sun inthe sky
cosmological principle
conjunction
Spectroscopic Parallax
Cassegrain Focus
40. Venus (retrograde)
quasar
open star clusters
slowest rotation
evidence of water on mars
41. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
coma
Dark Nebula
Flat - Remain Parallel - Exactly 1
Jovian Planets
42. Jupiter
Spectral Lines
Metals
Brown dwarf
Largest diameter
43. 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.
Void
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
superclusters
MOONS: most geologically active
44. A term referring to Jupiter-like planets
Autumnal Equinox
jovian
Hipparchus
Sc spiral galaxy
45. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
most moons
CNO Cycle
Spectroscopic Parallax
Gamma ray bursts
46. Is space infinitely large?
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47. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
Extrasolar Planet
Planetary Nebula
deferent
cosmic fireball
48. A location on an H-are Diagram where evolving stars pulsate
Instability strip
regolith
highlands
Ole Roemer
49. Wave- only waves cause an interference pattern when passing through a double slit - particle- only particles deposit energy at specific locations (the way an image builds up on digital camera)
Continuous Spectrum
Liquid metallic hydrogen
roche limit
Light: travels like a wave - detected like a particle
50. Europa
MOONS: roundest shape
belt
standard candle
Resolving Power