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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 gap etween saturn's A and B rings
roche limit
Cosmic Microwave Background
Cassini division
tectonics of Venus
2. Any class of objects with a uniform luminosity used to determine distance.
standard candle
cosmological principle
Heliocentric
300000 KM/sec
3. The 'edge' of the universe. Light beyond this has not reached us yet.
partile horizon
Heliocentric
Photosphere
Ground State
4. The measure of a variable star's apparent magnitude as it brightens and dims with time
Supercluster
Light Curve
meteoriod
Pixel
5. The temp at which a substance in the vacuum of space solidifies
Differential Rotation
AGN
MOONS: largest size
condensation temperature
6. 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.
era of recombination
dark energy
open star clusters
Metals
7. A word used in astronomy to describe all elements besides hydrogen and helium
mapping the structure of Milky Way disk
Neutron Star
Metals
force
8. The law that syas light energy from a blackbody increases as (temperature^4)
Vernal Equinox
Cosmic Microwave Background
Density Wave
Stephen-Boltzman Law
9. A subatomic particle with a negative charge. It creates light.
Autumnal Equinox
radiation dominated universe
dark matter
Electron
10. The force of attraction between any two objects having mass
gravity
radiation pressure
Rich vs poor clusters
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
11. The law that predicts the possible types of spectra.
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12. Neptune or uranus
Coldest surface
Parallax
Make up of the terrestrial planets
isotropic
13. The shadow area behind the Earth or Moon where the Sun is completely obscured.
Umbra
Inverse Square Law
Electron
blazar
14. Venus (retrograde)
Jupiters red spot
chondrite
slowest rotation
Molecular Clouds
15. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
cosmological principle
Thermonuclear Fusion
superclusters
disk
16. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Make up of the terrestrial planets
MOONS: larger than mercury
molecular clouds
Stephen-Boltzman Law
17. 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 ________.
Cosmic Microwave Background
scarp
Flat - Flat
hottest surface
18. Is there water on the moon?
Density Wave
Color Index
Flare
Yes - frozen at the poles- remains protected from the suns rays
19. Is there water on the moon?
Prominence
Granules
Yes - frozen at the poles- remains protected from the suns rays
Thickest atmosphere
20. A change in the wavelength of light caused by a motion between the observer and light (or wave) source (blue shift if getting closer - red shift if moving away)
Eclipses of the Moons of Jupiter
Doppler Shift
cosmological red shift
Electromagnetic Radiation: Radio
21. When material is heated and moves taking the heat energy with it
Convection
Poor Cluster
AGN
Chandrasekhar Limit
22. Stars fromt he Halo that have drifted into the disk. as earth zooms past them in a faster orbit they appear to be going backward very fast
High Velocity Stars
How is winding dilemma solved?
Electromagnetic Radiation: Infrared
Largest diameter
23. The surface of the sun
We don't know. It might be but does not have to be.
Photosphere
supermassive black hole
Kirkwood gaps
24. Infinitely long -> 10 cm
MOONS: thickest atmosphere
scarp
Molecular Clouds
Electromagnetic Radiation: Radio
25. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
aurora
shape and color of SPIRAL galaxies
quasar
tectonics of Earth
26. Star speed at outer edge of galaxy should begin to diminish - but they dont so we guess that this means there is increasing force (aka dark matter)
Thermonuclear Fusion
Active Optics
rotation curve = dark matter?
Metals
27. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
synchrotron radiation
radiation dominated universe
Rich vs poor clusters
Photon
28. A younger cluster of stars - found in the galaxy disk
Dwarf planets
Plank's Law
Open Cluster
general star population
29. Small compact stars called white dwarfs can have material deposited on their surfaces. In time material heats up and explodes in surface nuclear reaction- star brightens - settles - repeats.
Filament
accretion disk
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
nova
30. A fusion process in which protons build together to form helium
Globular Cluster
Proton-proton chain
differential rotation
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
31. The 'edge' of the universe. Light beyond this has not reached us yet.
partile horizon
Electron
Hydrostatic Equilibrium
Bok Globule
32. The family of radiant energy that includes light as a subset
Sunspot cycle
Precession
Europa (Jupiters moon)
Electromagnetic Radiation
33. The seasonal shifting of a nearby star's position relative to more distant objects.
meteor shower
Parallax
Granules
mare basalt
34. A star that is in the process of forming. It glows from gravitational contraction
Thermal Equilibrium
regolith
protostar
Spectral Lines
35. A star that is burning hydrogen to helium in a shell surrounding it's core
Cosmological Principle
radio lobe
Active Optics
Red Giant Branch Star
36. The gap inthe outer portion of Saturn's A ring
Enke gap
Oort Cloud
era of recombination
Nucleus
37. What are the three possible geometries of the universe?
Open - flat - and closed.
Terrestrial Planets
Blackbody
Sb spiral galaxy
38. Why do Galaxies move very rapidly in the interiors of the dense clusters?
How is winding dilemma solved?
Active Optics
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Heliocentric
39. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Make up of the terrestrial planets
Kirkwood gaps
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
tectonics of Earth
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)
quasar
greehouse effects
Ole Roemer
Milky way Galaxy
41. The lens that gathers the light in a refractor
critical density
Cosmic Microwave Background
Objective Lens
Hipparchus
42. The lowest energy of an atom.
Void
Europa (Jupiters moon)
great red spot
Ground State
43. The apparent path of the Sun through the stars on the celestial sphere.
300000 KM/sec
Ecliptic
Maria
Spectroscopic Parallax
44. A term referring to Jupiter-like planets
Autumnal Equinox
Europa (Jupiters moon)
jovian
Synodic Day
45. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
Dark Matter
Light Gathering Power
accretion disk
Geocentric
46. The part of the Milky way that has on-going star formation
3 reasons we orbit satellites to observe universe
Disk
Triple Alpha rocess
scarp
47. Sc galaxies
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
Flocculent spirals
Occam's razor
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.
48. 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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49. 10^2 nm 10^7 nm
Electromagnetic Radiation: Gamma Ray
Thickest atmosphere
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Hyashi track
50. A particle of light
Precession
How is winding dilemma solved?
Photon
meteor