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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 rotation of a star or planet at different speeds at its equator and poles
scarp
differential rotation
belt
Kirchhoff's Law
2. A method of finding a star's distance from its absolute magnitude and spectral type or color.
fusion crust
Hubble constant
Spectroscopic Parallax
OB Associations
3. A measure of the force of gravity on an object
Ammonia - methane - and water
Oort Cloud
weight
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.
4. 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.
open star clusters
Corona
nova
Poor Cluster
5. That which is responsible for Jupiter's magnetic field
Oort cloud
radiation pressure
differential rotation
Liquid metallic hydrogen
6. 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 _____.
Density Wave
Main Sequence Stars
Resolving Power
Flat - Remain Parallel - Exactly 1
7. The shadow area behind the Earth or Moon where the Sun is completely obscured.
difference between maria and highlands of the moon.
Cosmic Microwave Background (CMB)
density
Umbra
8. A bridge of material held in position above the solar surface. They can remain for hours even days
Prominence
radio galaxy
Filament
standard candle
9. The high- temperatature outer layer of the sun
Corona
Seyfert galaxy
deferent
Electromagnetic Radiation: Microwave
10. 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
Electromagnetic Radiation: Radio
radio lobe
Dwarf planets
Dark Nebula
11. A faint - remarkably uniform distribution of radiation in space
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
meteoriod
cosmic singularity
Cosmic Microwave Background
12. Mercury
thinnest atmosphere
Thermonuclear Fusion
Cosmological Principle
Galilean satellite
13. Light scattered through the atmosphere that degrades astronomical images
regolith
Colestial Pole
Light Pollution
cosmic fireball
14. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
nucleus
Negative - Diverge - Less than 1
supernova
gravity
15. A location on an H-are Diagram where evolving stars pulsate
cosmic singularity
Instability strip
Planck time
chemical differentiation
16. The projection of the Earth's equator onto the celestial sphere.
Apparent Magnitude
Jovian Planets
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Celestial Equator
17. A logarithmically scaled value for the measured brightness of a star.
Enke gap
Zenith
Apparent Magnitude
radio lobe
18. The rotation of a star or planet at different speeds at its equator and poles
differential rotation
cosmological principle
Photon
direct motion
19. The dark - relativley smooth areas on the moon; Latin for sea
solar nebula
Black Hole
Maria
Absorption Spectrum
20. 1 mm 1μm
Oort cloud
Electromagnetic Radiation: X-Ray
Electromagnetic Radiation: Infrared
The Big Bang Theory
21. When massive objects bend space and time enough to create multiple images of an object located behind them
partile horizon
Gravitational Lens
Umbra
force
22. The rotation period of the Earth measured relative to the Sun.
Colestial Pole
Synodic Day
Prominence
Plague
23. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
superclusters
3 reasons we orbit satellites to observe universe
Oort cloud
Coronal Loop
24. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Plank's Law
Negative - Diverge - Less than 1
Electromagnetic Radiation: Visible Light
chondrite
25. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Sb spiral galaxy
Make up of the terrestrial planets
Extrasolar Planet
Sa spiral galaxy
26. 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.
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.
Objective Lens
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
SETI
27. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Sc spiral galaxy
Big Bang
Open - flat - and closed.
Ammonia - methane - and water
28. 10 nm 10^2 nm
Electromagnetic Radiation: X-Ray
Proton-proton chain
How is winding dilemma solved?
radiant
29. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
superclusters
Photometry
planetary nebula
quasar
30. A galaxy sending out a stream of material from its nucleus
Radio Galaxy
Spectroscopic Parallax
regolith
Cosmic Microwave Background (CMB)
31. 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.
nova
A family of radiant energy- includes light
Shepherd satellite
Halo
32. Ganymede
density parameter
MOONS: largest size
contrast northern lowlands and the southern highlands of mars...
Cassegrain Focus
33. A galaxy sending out a stream of material from its nucleus
radiant
Radio Galaxy
inferior planets
supermassive black hole
34. Hot cells of gas that rise and fall in the hotosphere
Halo
Milky way Galaxy
Electromagnetic Radiation: Visible Light
Granules
35. Venus
shape and color of ELLIPTICAL galaxies
superclusters
hottest surface
Kirchhoff's Law
36. What do we think the actual fate of the universe will be and why do we think this?
Electromagnetic Radiation: Microwave
Self-Propogating Star Formation
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.
Gravitational Lens
37. Is there water on the moon?
Radio Galaxy
Yes - frozen at the poles- remains protected from the suns rays
solar nebula
Electromagnetic Radiation: Gamma Ray
38. A representation of the changes in color and brightness of an evolving protostar.
Hyashi track
Flocculent spirals
Metals
chondrite
39. 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 ________.
disk
3 reasons we orbit satellites to observe universe
Flat - Flat
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
40. The equation that describes how matter equates with energy
Thermal Equilibrium
High Velocity Stars
E=mc2
Most dense
41. Europa
Meridian
MOONS: roundest shape
era of recombination
Self-Propogating Star Formation
42. The imaginary sphere centered on the Earth that hols the stars.
shape and color of SPIRAL galaxies
Celestial Sphere
Primary Mirror
Inverse Square Law
43. A telescope that uses lenses to focus light
Refractor
semimajor axis
Thickest atmosphere
rotation curve=winding dilemma?
44. A measure of the force of gravity on an object
weight
Flat - Flat
smallest diameter
Seyfert galaxy
45. The north-south line passing directly overhead through the zenith.
Meridian
Globular Cluster
mapping the structure of Milky Way disk
solar nebula
46. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
self-propagating star formation
Spectroscopic parallax
AGN
Electromagnetic Radiation
47. The temp at which a substance in the vacuum of space solidifies
self-propagating star formation
condensation temperature
CMB
synchronous rotation
48. The gap inthe outer portion of Saturn's A ring
Cassegrain Focus
CMB
Enke gap
planetesimal
49. 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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50. In what chemical form are jupiters nitrogen - carbon and oxygen?
MOONS: larger than mercury
Molecular Clouds
Ammonia - methane - and water
Titus-Bode Law