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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 linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
Oort Cloud
Hubble law
We don't know. It might be but does not have to be.
cosmological red shift
3. Light-colored high-pressure bands in Jupiter's atmosphere
AGN
Negative - Diverge - Less than 1
zone
Inverse Square Law
4. A long-lived high-pressure bulge in Jupiter's southern hemisphere
Red Giant Branch Star
Umbra
cosmological red shift
great red spot
5. The distance light travels in one year (=9.46x10^12km).
Light-Year
Cosmic Microwave Background
Parallax
Chandrasekhar Limit
6. The faint glow of light left over from the Big Bang. cosmic microwave background are the photons that remain after the big bang that have not turned into matter.
most eccentric orbit
CMB
Seyfert galaxy
Ionization
7. 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)
Planck time
Gamma ray bursts
Cepheid Variable
Electromagnetic Radiation
8. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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9. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Maria
Absolute Magnitude
Hubble constant
tectonics of Venus
10. A star fusing hydrogen to helium in it's core
opposition
Sa spiral galaxy
Main Sequence Stars
CMB
11. The gap inthe outer portion of Saturn's A ring
evidence of water on mars
bulge
Rich Cluster
Enke gap
12. The oldest grouping of stars - found in the galaxy halo
Primary Mirror
jovian
H2 Regions
Globular Cluster
13. The larger bodies that formed early in teh solar nebula that were chemically differentiated
Light-Year
tectonics of Mars
planetesimal
Meridian
14. The mirror that determines the focus configuration of a reflector
critical density
Secondary Mirror
Gamma ray bursts
asteroid
15. Long - meandering cliff formed when a planet surface cools and shrinks
scarp
Parallax
Electron
Resolving Power
16. The place in the sky that the Earth's axis points toward (can be either north or south)
Seeing
Colestial Pole
Inverse Square Law
Pixel
17. The part of the Milky way that has on-going star formation
mass
Disk
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Electromagnetic Radiation: Radio
18. 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.
Particle Horizon
contrast northern lowlands and the southern highlands of mars...
If it is in a denser medium - such as glass - it will move slower
Refractor
19. The point in its orbit where a planet is farthest from the sun
Electromagnetic Radiation: Radio
aphelion
Bulge
matter dominated universe
20. When one side of a body always faces the planet it revolves around
Coronal Loop
synchronous rotation
Primary Mirror
Sc spiral galaxy
21. Distribution of dust (tells us disk is thin) - find distances to O&B stars and H2 regions (arms are sights of star formation and OB stars live and die at location of birth) -Milky way has four arms. Sun is in spur apart from arms.
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
mapping the structure of Milky Way disk
300000 KM/sec
Eclipses of the Moons of Jupiter
22. Matter that reveals itself only through its gravitational attraction.
Main Sequence Stars
dark matter
self-propagating star formation
Shepherd satellite
23. The oldest terrain on the moon
Shepherd satellite
highlands
Planetary Nebula
Ecliptic
24. When massive objects bend space and time enough to create multiple images of an object located behind them
Flare
Shepherd satellite
great red spot
Gravitational Lens
25. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Halo
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.
radiation dominated universe
CCD
26. The telescope configuration that has the focus placed at the back of the primary mirror
Cassegrain Focus
tectonics of Venus
Turn off Point
mare basalt
27. The gap etween saturn's A and B rings
Sc spiral galaxy
chemical differentiation
300000 KM/sec
Cassini division
28. A prominence seen against the disk of the sun
Filament
Eyepiece Lens
Resolving Power
most moons
29. Then the Sun moves from north to south across the celestial equator (about September 23)
Autumnal Equinox
Ground State
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.
density
30. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Gamma ray bursts
Negative - Diverge - Less than 1
zone
roche limit
31. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Ganymede (Jupiter)
Ammonia - methane - and water
condensation temperature
Spectral Lines
32. Europa
Stephen-Boltzman Law
most moons
Kuiper belt
MOONS: roundest shape
33. 10 nm 10^2 nm
Big Bang
Hubble law
Electromagnetic Radiation: X-Ray
Autumnal Equinox
34. 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.
contrast northern lowlands and the southern highlands of mars...
quasar
Maria
isotropic
35. A volume of space where few - if any - galaxies are located
contrast northern lowlands and the southern highlands of mars...
gravity
fewest moons
Void
36. A telescope that uses mirrors to focus light
High Velocity Stars
Primary Mirror
Reflector
A family of radiant energy- includes light
37. A small chunk of rock in space
shape and color of SPIRAL galaxies
Chandrasekhar Limit
Absolute Magnitude
meteoriod
38. 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)
Doppler Shift
Electromagnetic Radiation
Instability strip
quasar
39. Clouds of low density gas often found glowing faintly on either side of an AGN.
Photometry
radio lobe
Pixel
Cassini division
40. The dark - relativley smooth areas on the moon; Latin for sea
Cepheid Variable
Prominence
Maria
Refractor
41. What causes the zones and belts on jupiter and saturn?
MOONS: larger than mercury
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
Total Eclipse
High Velocity Stars
42. Hot cells of gas that rise and fall in the hotosphere
Milky way Galaxy
Granules
neutrino
Electromagnetic Radiation
43. Why does the earth have few craters while the moon has many?
accretion disk
cosmological principle
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Convection
44. Venus
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
Chromosphere
hottest surface
zone
45. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Oort cloud
Focal Length
Void
slowest rotation
46. The source of the force that is accelerating the expansion rate of the universe.
300000 KM/sec
cosmological red shift
dark energy
Spectroscopic Parallax
47. A measure of the ability of a telescope to see fine detail
Flare
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
radio lobe
Resolving Power
48. A spread of light with an uninterrupted wavelength distribution of energy.
Density Wave
Continuous Spectrum
Jupiters red spot
Filament
49. Ganymede and Titan
partile horizon
MOONS: larger than mercury
Horizontal Branch Star
Ole Roemer
50. Large nebula consisting of very cold gas and dust
quasar
Molecular Clouds
Ionization
dark matter