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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 location on an H-are Diagram where evolving stars pulsate
Instability strip
Self-Propogating Star Formation
cosmology
opposition
2. Venus
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Cepheid variables
Roundest orbit
Convection
3. The act of removing an electron from an atom.
Astronomical Unit
Ionization
Coronal Loop
Light Gathering Power
4. The average distance between the Earth and the Sun (=1.5 x10^8km)
Winter Solstice
shape and color of SPIRAL galaxies
CMB
Astronomical Unit
5. The oldest grouping of stars - found in the galaxy halo
acceleration
CMB
most moons
Globular Cluster
6. Light-colored high-pressure bands in Jupiter's atmosphere
MOONS: largest size
zone
Planetary Nebula
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.
7. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
rotation curve=winding dilemma?
Absolute Magnitude
tectonics of Mars
cosmic singularity
8. A star that has become a red giant for the second and final time. It is burning helium to carbon in a shell surrounding the core
Asymptotic giant Branch Star
most eccentric orbit
condensation temperature
supernova
9. The state of having a balance between inward and outard pressures in a gas--the inward force from gravity is balanced by the outward force from heat.
Hydrostatic Equilibrium
Quasar
Supercluster
Thickest atmosphere
10. The powdered stone fragments that make up the lunar 'soil'
Penumbra
epicycle
Gravitational Lens
regolith
11. 10^2 nm 10^7 nm
protostar
most moons
Electromagnetic Radiation: Gamma Ray
Grand design spirals
12. Flat disk with gas - dust - H2 regions - molecular clouds - dust young stars and remnants of old planetary nebula and supernova remnants. stars spin together with similar velocities called differential rotation
self-propagating star formation
conjunction
disk
CMB
13. The location around an atom where an electron resides.
Oort cloud
cosmic fireball
jovian
Energy Level
14. The high- temperatature outer layer of the sun
CNO Cycle
resonance
Geocentric
Corona
15. The number of protons in an atom.
Void
Corona
Atomic Number
Electromagnetic Radiation: Microwave
16. The class of all objects having high energy radiation coming from their nuclei. Active Galactic Nucleus- Blazars - Quasars - Radio and Emit synchrotron radiation
Synchrotron Rotation
Instability strip
AGN
Parallax
17. Why does the earth have few craters while the moon has many?
Cassini division
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
MOONS: larger than mercury
Electromagnetic Radiation
18. Elliptical orbits that come inside orbit of the Earth.
Apollo asteroids
meteor
direct motion
White Dwarf
19. How is the Hubble Law consistent with an expanding universe?
Turn off Point
great red spot
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.
Ecliptic
20. The force of attraction between any two objects having mass
molecular clouds
gravity
Gravitational Lens
Total Eclipse
21. The law that predicts the possible types of spectra.
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22. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
mass
accretion disk
Heliocentric
greatest elongation
23. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
general star population
Gamma ray bursts
Negative - Diverge - Less than 1
rotation curve = dark matter?
24. Hydrogen and helium (mainly)
planetesimal
Galilean satellite
Make up of the jovian planets
greehouse effects
25. A volume of space where few - if any - galaxies are located
Synchrotron Rotation
Void
Coldest surface
Cassini division
26. The Greek philosopher responsible for making the stellar magnitude scale.
Particle Horizon
meteor
Hipparchus
Neutron Star
27. When material is heated and moves taking the heat energy with it
Coldest surface
E=mc2
Cepheid Variable
Convection
28. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Quasar
radiation dominated universe
Continuous Spectrum
AGN
29. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Bok Globule
Flocculent spirals
Open - flat - and closed.
Absolute Magnitude
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____.
Sc spiral galaxy
synchronous rotation
Negative - Diverge - Less than 1
differential rotation
31. A two-filter measure of the color - and hence temperature - of a star.
planetesimal
Color Index
chemical differentiation
Plank's Law
32. A location on an H-are Diagram where evolving stars pulsate
Instability strip
A family of radiant energy- includes light
Pixel
Atomic Number
33. What causes the zones and belts on jupiter and saturn?
tectonics of Venus
Big Bang
Rich Cluster
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
34. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Halo
direct motion
Resolving Power
Main Sequence
35. A very dense - highly populated cluster of galaxies
Rich Cluster
Big Bang
How is winding dilemma solved?
Light-Year
36. A quantity measuring the stability of the Earth's atmosphere
Instability strip
Stephen-Boltzman Law
mare basalt
Seeing
37. Mercury and venus
fusion crust
fewest moons
mass
Poor Cluster
38. A massive variable star used to find distances to the galaxies or clusters that contain them.
Cepheid Variable
aurora
Colestial Pole
tectonics of Mars
39. 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)
How is winding dilemma solved?
thinnest atmosphere
radio galaxy
Photon
40. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Rich vs poor clusters
Kirkwood gaps
Halo
smallest diameter
41. Venus (retrograde)
slowest rotation
Extrasolar Planet
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.
zone
42. Mercury - Venus - Earth - Mars
Terrestrial Planets
regolith
Photon
Hubble law
43. A point in the sky where meteors appear to come from during a shower
Wein's Law
radiant
Largest diameter
Meridian
44. The location of a supermassive black hole
Nucleus
Electromagnetic Radiation: Gamma Ray
Pulsar
supernova
45. 10^2 nm 10^7 nm
comet
HII Region
Electromagnetic Radiation: Gamma Ray
Dwarf planets
46. A very dense - highly populated cluster of galaxies
Pulsar
density waves
Rich Cluster
Synodic Day
47. Small moons that maintain the shape of rings around Saturn and Uranus
Annular Eclipse
Interstellar Extinction
protostar
Shepherd satellite
48. The layer of the sun just above the photosphere
Chromosphere
MOONS: most geologically active
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.
Kirkwood gaps
49. The measure of a variable star's apparent magnitude as it brightens and dims with time
Parallax
We don't know. It might be but does not have to be.
Lagrangian Razor
Light Curve
50. An evolved star - past the helium flash that is burning helium to carbon in it's cores
Electromagnetic Radiation: Infrared
Color Index
Coldest surface
Horizontal Branch Star