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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. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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2. The rotation period of the Earth measured relative to the Sun.
Synodic Day
Radio Galaxy
Shepherd satellite
disk
3. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
Photon
self-propagating star formation
Asymptotic giant Branch Star
Electromagnetic Radiation
4. A rock or iron specimen that has fallen from space
most moons
Galilean satellite
density parameter
meteorite
5. The place in the sky that the Earth's axis points toward (can be either north or south)
fewest moons
Electromagnetic Radiation: Infrared
Parallax
Colestial Pole
6. 1μm 100 nm
Cosmic Microwave Background (CMB)
Europa (Jupiters moon)
Hubble law
Electromagnetic Radiation: Visible Light
7. 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.
Photon
MOONS: larger than mercury
CNO Cycle
Jupiters red spot
8. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
Triple Alpha rocess
E=mc2
Light Pollution
Planck time
9. The process that powers the sun and hydrogen bombs
Nova
radiation dominated universe
Thermonuclear Fusion
Electromagnetic Radiation: Visible Light
10. The lens in a telescope used to determine the magnification
Plague
Europa (Jupiters moon)
Eyepiece Lens
density waves
11. The distance a moon can be from a planet before shattering from tidal forces
Rich vs poor clusters
roche limit
Parallax
radio galaxy
12. All possible types of energy that can be emitted and absorbed by atoms.
Pixel
Electromagnetic Radiation
H-are Diagram
scarp
13. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Eclipses of the Moons of Jupiter
Yes - frozen at the poles- remains protected from the suns rays
tectonics of Earth
Gravitational Lens
14. The distance a moon can be from a planet before shattering from tidal forces
roche limit
Kirchhoff's Law
force
Light Pollution
15. A measure of the seasonal shifting of a star's position against farther stars or galaxies. The closer the star - the greater is the angular distance it shifts. We use it to find distances to stars that are up to 1000 pc away.
Parallax
Photon
Absorption Spectrum
conjunction
16. When the Sun is farthest north of the celestial equator (about June 22)
H-are Diagram
quasar
Yes - frozen at the poles- remains protected from the suns rays
Summer Solstice
17. The Greek philosopher responsible for making the stellar magnitude scale.
Enke gap
Hipparchus
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
Trojan asteroids
18. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Spectral Lines
Bulge
Nebula
gravity
19. A particle of light.
molecular clouds
Main Sequence Stars
shape and color of ELLIPTICAL galaxies
Photon
20. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Active Optics
aphelion
Olber's paradox
chemical differentiation
21. The name for the only seriously considered theory of the universe.
Ground State
Big Bang
Penumbra
Rich Cluster
22. Approximate speed of light in a vacuum
Cepheid variables
Kirkwood gaps
Instability strip
300000 KM/sec
23. A plot of star absolute magnitude verses spectral type.
hottest surface
A family of radiant energy- includes light
H-are Diagram
nova
24. The area behind a lens where images are resolved
Photosphere
Focal Plane
meteor shower
nova
25. A term referring to the orbital character of stars near the Sun
difference between maria and highlands of the moon.
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
Differential Rotation
Heliocentric
26. When a planet lines up with the sun inthe sky
Asymptotic giant Branch Star
conjunction
Electromagnetic Radiation: Infrared
quarks
27. VENUS
density waves
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
slowest rotation
Dark Matter
28. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Absolute Magnitude
OB Associations
Jupiters red spot
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.
29. First accurately measured the speed of light in a vacuum
Electromagnetic Radiation: Visible Light
Geocentric
Ole Roemer
Nebula
30. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Sb spiral galaxy
tectonics of Earth
31. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
quasar
Oort cloud
Open Cluster
roche limit
32. The organization of clusters of galaxies into sheets and strings
HII Region
Gamma-ray Burst
Supercluster
CMB
33. What do we think the actual fate of the universe will be and why do we think this?
Radio Galaxy
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.
Photon
mapping the structure of Milky Way disk
34. A change in the appearance of the sun at the edge of the solar disk
Nova
Sa spiral galaxy
Limb darkening
Halo
35. Long - meandering cliff formed when a planet surface cools and shrinks
scarp
Prominence
Electromagnetic Radiation: Gamma Ray
Cosmological Principle
36. Matter so dense that even light cannot escape its gravity
Black Hole
Open Cluster
Seeing
general star population
37. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
dark energy
Main Sequence
Radiative Diffusion
plate tectonics
38. 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.
Ground State
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Gravitational Lens
coma
39. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Sc spiral galaxy
Asymptotic giant Branch Star
Penumbra
tectonics of Earth
40. A star that is in the process of forming. It glows from gravitational contraction
Globular Cluster
supernova
Electromagnetic Radiation
protostar
41. When the Sun is farthest south of the celestial equator (About December 22)
quasar
Winter Solstice
Ionization
cosmology
42. The family of radiant energy that includes light as a subset
radiation dominated universe
conjunction
Maria
Electromagnetic Radiation
43. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
difference between maria and highlands of the moon.
Chromosphere
Cassini division
radiation dominated universe
44. Saying that the sky should not get dark at night because all lines of sight end on a star meaning that the night sky should be ablaze BUT the big bang - because the universe had a beginning - says that the sky gets dark because out in space - galaxie
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45. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
Active Optics
Rich Cluster
Cosmic Microwave Background (CMB)
density parameter
46. An energetic event taking place in the early universe
Gamma-ray Burst
Convection
E=mc2
Hubble constant
47. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Electromagnetic Radiation: Gamma Ray
Asymptotic giant Branch Star
Absorption Spectrum
Photometry
48. The mirror that determines the focus configuration of a reflector
epicycle
Hubble constant
widmanstatten pattern
Secondary Mirror
49. The family of radiant energy that includes light as a subset
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
Drake equation
Largest diameter
Electromagnetic Radiation
50. 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.
Oort Cloud
differential rotation
Bulge
The Big Bang Theory