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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. A small spherical dark nebula
Photosphere
Bok Globule
Wein's Law
We don't know. It might be but does not have to be.
2. How did Earth come to have an oxygen rich atmosphere?
Bok Globule
Grand design spirals
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.
Photon
3. A continuous spectrum of light missing energy at a few wave lengths.
coma
aphelion
Absorption Spectrum
radiant
4. The mix of pure photon energy that emerged at the start of the universe.
radio lobe
Flat - Remain Parallel - Exactly 1
Population 1 vs Population 2 stars
cosmic fireball
5. When a planet lines up with the sun inthe sky
Superior planets
zone
conjunction
Light Curve
6. The area behind a lens where images are resolved
Thermonuclear Fusion
inferior planets
Neutron Star
Focal Plane
7. The process similar to conduction by which energy moves from the solar core to the convective layer
Radiative Diffusion
thinnest atmosphere
Electromagnetic Radiation: X-Ray
Turn off Point
8. Large nebula consisting of very cold gas and dust
HII Region
meteor
Black Hole
Molecular Clouds
9. The number of protons in an atom.
Atomic Number
3 reasons we orbit satellites to observe universe
meteor
Coldest surface
10. Any change in the speed or direction of an object's motion
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.
acceleration
critical density
Electromagnetic Radiation: Infrared
11. The surface of the sun
Cassegrain Focus
Sa spiral galaxy
Photosphere
least dense
12. The material from which the solar system formed
Yes - frozen at the poles- remains protected from the suns rays
solar nebula
interstellar dust
Light: travels like a wave - detected like a particle
13. The era when the ratio of matter to energy greatly favored matter. (verses radiation dominated universe where it was opaque. Matter is now dominated by gravity not photons)
matter dominated universe
Planetary Nebula
Seyfert galaxy
Coronal Loop
14. Titan
Callisto (Jupiter)
Sc spiral galaxy
Gamma-ray Burst
MOONS: thickest atmosphere
15. Any change in the speed or direction of an object's motion
Maria
Oort Cloud
acceleration
fewest moons
16. A fusion process in which protons build together to form helium
Proton-proton chain
Refractor
Planetary Nebula
greehouse effects
17. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
Self-Propogating Star Formation
Planck time
bulge
Kuiper belt
18. The location in an H-are diagram of a star cluster - where stars have just left the main sequence. Used to estimate the cluster age.
chemical differentiation
Turn off Point
Make up of the jovian planets
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
19. A logarithmically scaled value for the measured brightness of a star.
force
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.
Apparent Magnitude
epicycle
20. A spectrum of light with energy at only a few wavelengths.
Oort cloud
Emission Spectrum
Coldest surface
Electromagnetic Radiation
21. Saturn
Apollo asteroids
least dense
opposition
Photon
22. Centered on the Earth
Geocentric
Shepherd satellite
Ecliptic
smallest diameter
23. Jupiter
Chandrasekhar Limit
We don't know. It might be but does not have to be.
Winter Solstice
Largest diameter
24. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
plate tectonics
Ammonia - methane - and water
evidence of water on mars
quasar
25. A push or a pull
Electromagnetic Radiation: X-Ray
force
Planck time
Spectroscopic Parallax
26. Matter so dense that even light cannot escape its gravity
Black Hole
Oort cloud
CNO Cycle
Precession
27. A planet that is closer to the sun than the earth
Red Giant
Electromagnetic Radiation: Radio
inferior planets
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
28. The force of attraction between any two objects having mass
Instability strip
Ole Roemer
gravity
shape and color of ELLIPTICAL galaxies
29. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Spectroscopic Parallax
Make up of the terrestrial planets
Callisto (Jupiter)
radio lobe
30. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Ecliptic
Main Sequence
Nucleus
most eccentric orbit
31. The lens in a telescope used to determine the magnification
deferent
Color Index
Galilean satellite
Eyepiece Lens
32. The oldest part of the Milky Way
radio galaxy
Halo
Reflector
jovian
33. The time when the universe cooled sufficiently for atoms to exist. radiation dominated= first 300000 years - THEN era of recombination turns into matter dominated for next.
Sidereal Day
anorthosite
era of recombination
Electromagnetic Radiation: Microwave
34. The source of the force that is accelerating the expansion rate of the universe.
asteroid
Triple Alpha rocess
Seyfert galaxy
dark energy
35. 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
Bulge
Steady State Theory (Leads to Olber's Paradox)
A family of radiant energy- includes light
Hubble law
36. Loops that trace the magnetic field as it erupts from a sunspot area and arches over to an adjacent area. They glow in the light of gas pouring out of corona and falling into photosphere.
synchronous rotation
Sunspot cycle
anorthosite
Coronal Loop
37. Jupiter
Enke gap
Total Eclipse
great red spot
fastest rotation
38. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
cosmological principle
tectonics of Venus
Precession
White Dwarf
39. Matter that reveals itself only through its gravitational attraction
Dark Matter
Sc spiral galaxy
Synchrotron Rotation
radiation pressure
40. 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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41. The rotation of a star or planet at different speeds at its equator and poles
Black Hole
differential rotation
radiation dominated universe
Photometry
42. A measure of the force of gravity on an object
Most dense
weight
Asymptotic giant Branch Star
Dark Nebula
43. The location around an atom where an electron resides.
Spectral Lines
radio galaxy
Energy Level
quasar
44. The rate of expansion of the universe.
Rich vs poor clusters
Hubble constant
radiation dominated universe
Oort cloud
45. Moon in less than the angular diameter of the Sun.
Limb darkening
Annular Eclipse
Halo
MOONS: larger than mercury
46. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
chondrite
cosmological principle
Superior planets
asteroid
47. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Celestial Equator
tectonics of Earth
Rich vs poor clusters
Largest diameter
48. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Resolving Power
critical density
shape and color of ELLIPTICAL galaxies
blazar
49. The process that powers the sun and hydrogen bombs
Thermonuclear Fusion
Rich Cluster
Thermal Equilibrium
dark energy
50. 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
Apparent Magnitude
Electromagnetic Radiation: Infrared
dark energy
Hubble law