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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 line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Inverse Square Law
Main Sequence
belt
cosmic singularity
2. A force exerted by reflecting sunlight
Chromosphere
Blackbody Curve
cosmological red shift
radiation pressure
3. Mercury
radiation dominated universe
density
Absorption Spectrum
smallest diameter
4. The temp at which a substance in the vacuum of space solidifies
condensation temperature
MOONS: roundest shape
MOONS: larger than mercury
We don't know. It might be but does not have to be.
5. VENUS
Asymptotic giant Branch Star
Celestial Sphere
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
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
6. A term referring to the orbital character of stars near the Sun
interstellar dust
Absolute Magnitude
Differential Rotation
Active Optics
7. Why does the earth have few craters while the moon has many?
Brown dwarf
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Thermal Equilibrium
Absorption Spectrum
8. A telescope that uses mirrors to focus light
HII Region
Reflector
Flat - Flat
Particle Horizon
9. When one side of a body always faces the planet it revolves around
synchronous rotation
meteoriod
difference between maria and highlands of the moon.
Cosmological Principle
10. Centered on the Earth
greatest elongation
Geocentric
nucleus
retrograde motion
11. Hot cells of gas that rise and fall in the hotosphere
Metals
asteroid
Granules
Absorption Spectrum
12. 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.
rotation curve=winding dilemma?
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Oort Cloud
Eyepiece Lens
13. Stars orvits do not define the spiral patterns - instead they are density waves that move at slower speeds (arms are defined by young O and B stars and gas clouds)
Light Curve
density parameter
How is winding dilemma solved?
E=mc2
14. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
Summer Solstice
standard candle
accretion disk
Density Wave
15. Matter that reveals itself only through its gravitational attraction.
How is winding dilemma solved?
Flat - Flat
nova
dark matter
16. A spectrum of light with energy at only a few wavelengths.
Emission Spectrum
quasar
great dark spots
Drake equation
17. The measure of a variable star's apparent magnitude as it brightens and dims with time
solar nebula
HII Region
Light Curve
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.
18. A huge sphere of tenuous gas surrounding the nucleus of a comet
Photon
condensation temperature
coma
Molecular Clouds
19. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Asymptotic giant Branch Star
Asymptotic giant Branch Star
CNO Cycle
general star population
20. Form honeycomb like patterns surrounding empty or nearly empty voids.
superclusters
widmanstatten pattern
Superior planets
Supercluster
21. 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
Void
bulge
Main Sequence Stars
Apparent Magnitude
22. Is space infinitely large?
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23. Ganymede
Dark Nebula
tectonics of Earth
MOONS: largest size
CCD
24. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
Rich Cluster
deferent
Negative - Diverge - Less than 1
density parameter
25. 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.
Electromagnetic Radiation: Radio
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
open star clusters
density waves
26. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Autumnal Equinox
Flare
molecular clouds
least dense
27. Electromagnetic Radiation
The Local Group
scarp
A family of radiant energy- includes light
Refractor
28. A collection of comets in the plane of the solar system - located beyond the orbit of Pluto
most eccentric orbit
Kuiper belt
MOONS: largest size
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.
29. A planet that is closer to the sun than the earth
inferior planets
Continuous Spectrum
cosmological principle
Electromagnetic Radiation: Gamma Ray
30. What Ole Roemer used to measure the speed of light in a vacuum
condensation temperature
slowest rotation
Eclipses of the Moons of Jupiter
Hydrostatic Equilibrium
31. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
Ammonia - methane - and water
conjunction
radio galaxy
greehouse effects
32. Large nebula consisting of very cold gas and dust
direct motion
Blackbody Curve
Molecular Clouds
Make up of the jovian planets
33. Long - meandering cliff formed when a planet surface cools and shrinks
great red spot
scarp
Astronomical Unit
Differential Rotation
34. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
H-are Diagram
Callisto (Jupiter)
Supercluster
Cepheid Variable
35. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Proton-proton chain
nucleus
Thermal Equilibrium
AGN
36. The larger bodies that formed early in teh solar nebula that were chemically differentiated
Oort cloud
Red Giant
planetesimal
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
37. The elementary building blocks from which protons and neutrons are formed.
nova
Proton-proton chain
Refractor
quarks
38. Moon in less than the angular diameter of the Sun.
Annular Eclipse
Dark matter candidates
shape and color of SPIRAL galaxies
Spectral Lines
39. The source of the force that is accelerating the expansion rate of the universe.
matter dominated universe
Thickest atmosphere
dark energy
Umbra
40. A galaxy emitting large amounts of energy at long wavelengths.
supermassive black hole
Sa spiral galaxy
radio galaxy
Penumbra
41. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Asymptotic giant Branch Star
3 reasons we orbit satellites to observe universe
Supercluster
Bulge
42. The point directly overhead.
plate tectonics
E=mc2
Zenith
Bok Globule
43. A star that blows itself apart
Supernova (You can be my supernova girl)
Bulge
Main Sequence
density waves
44. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
accretion disk
Drake equation
Trojan asteroids
synchrotron radiation
45. A faint - remarkably uniform distribution of radiation in space
cosmological principle
Sidereal Day
Cosmic Microwave Background
Light Pollution
46. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Radio Galaxy
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
coma
Absolute Magnitude
47. Titan
nova
mass
Continuous Spectrum
MOONS: thickest atmosphere
48. The family of radiant energy that includes light as a subset
Metals
Electromagnetic Radiation
thinnest atmosphere
Supercluster
49. Norhern lowlands- darker in color and have far fewer craters as if an ancient sea or ice field covered them. southern highlands- much higher in density of craters.
superclusters
Hubble law
Energy Level
contrast northern lowlands and the southern highlands of mars...
50. Jupiter
most moons
rotation curve=winding dilemma?
quasar
Supernova (You can be my supernova girl)