SUBJECTS
|
BROWSE
|
CAREER CENTER
|
POPULAR
|
JOIN
|
LOGIN
Business Skills
|
Soft Skills
|
Basic Literacy
|
Certifications
About
|
Help
|
Privacy
|
Terms
|
Email
Search
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. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
great dark spots
density
Reflector
tectonics of Earth
2. A force exerted by reflecting sunlight
radiation pressure
Molecular Clouds
HII Region
fewest moons
3. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
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.
Limb darkening
If it is in a denser medium - such as glass - it will move slower
Celestial Sphere
4. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
tectonics of Mars
Coronal Loop
Cosmic Microwave Background
Summer Solstice
5. Electromagnetic Radiation
Refractor
Summer Solstice
A family of radiant energy- includes light
MOONS: thickest atmosphere
6. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Ammonia - methane - and water
rotation curve=winding dilemma?
differential rotation
Disk
7. Centered on the Earth
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
Geocentric
Plank's Law
Globular Cluster
8. Hydrogen and helium (mainly)
Make up of the jovian planets
Autumnal Equinox
Milky way Galaxy
roche limit
9. Is there water on the moon?
Turn off Point
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Kirkwood gaps
Yes - frozen at the poles- remains protected from the suns rays
10. Then the Sun moves from north to south across the celestial equator (about September 23)
Hipparchus
Supernova (You can be my supernova girl)
Chandrasekhar Limit
Autumnal Equinox
11. A term referring to the orbital character of stars near the Sun
Differential Rotation
critical density
Zenith
Parallax
12. That which is responsible for Jupiter's magnetic field
Callisto (Jupiter)
Liquid metallic hydrogen
radiant
homogeneous
13. Neptune or uranus
Blackbody Curve
Kuiper belt
Shepherd satellite
Coldest surface
14. Venus
hottest surface
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.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Rich Cluster
15. Dark - reddish - low-pressure bands in Jupiter's atmosphere
Titus-Bode Law
belt
Apparent Magnitude
Dark Nebula
16. Half of the longest diameter across an ellipse
Seeing
Summer Solstice
Atomic Number
semimajor axis
17. The high- temperatature outer layer of the sun
fusion crust
Corona
deferent
Jupiters red spot
18. The relation that tells how light dims with distance.
Inverse Square Law
Dark Matter
Pulsar
Stephen-Boltzman Law
19. A small round distribution of gas surrounding a dying star
Planetary Nebula
Sb spiral galaxy
self-propagating star formation
Big Bang
20. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
greehouse effects
Supernova (You can be my supernova girl)
Spectroscopy
Molecular Clouds
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.
Electromagnetic Radiation: Gamma Ray
Void
blazar
mapping the structure of Milky Way disk
22. A small spherical dark nebula
Seyfert galaxy
Bok Globule
Inverse Square Law
self-propagating star formation
23. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
nucleus
Continuous Spectrum
Rich vs poor clusters
belt
24. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
Milky way Galaxy
Precession
Annular Eclipse
tectonics of Mars
25. 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
bulge
tectonics of Venus
Magnification
Big Crunch
26. The lens in a telescope used to determine the magnification
Black Hole
Most dense
jovian
Eyepiece Lens
27. A measure of the seasonal shifting of a star's position against farther stars or galaxies. The closer the star - the greater is the angular distance it shifts. We use it to find distances to stars that are up to 1000 pc away.
Light-Year
Hubble law
Spectroscopy
Parallax
28. What causes the zones and belts on jupiter and saturn?
fusion crust
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
Brown dwarf
Kuiper belt
29. The shadow area behind the Earth or Moon where the Sun is completely obscured.
MOONS: roundest shape
Cassini division
Thickest atmosphere
Umbra
30. A star that is in the process of forming. It glows from gravitational contraction
Celestial Equator
matter dominated universe
great dark spots
protostar
31. Collections of young - hot stars
OB Associations
Primary Mirror
self-propagating star formation
Total Eclipse
32. The gap etween saturn's A and B rings
Cassini division
chemical differentiation
Molecular Clouds
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.
33. Either Io -Europa - Ganymede - or Callisto
Galilean satellite
Ganymede (Jupiter)
Open Cluster
Sunspots
34. The law that describes the blackbody curve - and let to quantum mechanics.
Warning
: Invalid argument supplied for foreach() in
/var/www/html/basicversity.com/show_quiz.php
on line
183
35. A spectrum of light with energy at only a few wavelengths.
Photon
Emission Spectrum
Particle Horizon
cosmology
36. An energetic event taking place in the early universe
Gamma-ray Burst
Light Curve
Red Giant
Rich vs poor clusters
37. A distance measure determined by the shifting of a star against the background sky every 6 months.
Parsec
anorthosite
Triple Alpha rocess
Continuous Spectrum
38. The family of radiant energy that includes light as a subset
Oort Cloud
acceleration
Electromagnetic Radiation
High Velocity Stars
39. All wavelengths of light emitted by a blackbody.
Roundest orbit
regolith
Milky way Galaxy
Blackbody Curve
40. A volume of space where few - if any - galaxies are located
Instability strip
Void
Disk
semimajor axis
41. How did Earth come to have an oxygen rich atmosphere?
nova
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.
Electromagnetic Radiation
quarks
42. Earth
Most dense
fusion crust
radio galaxy
nucleus
43. 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?
Io (jupiters moon)
tectonics of Mars
meteor shower
44. All possible types of energy that can be emitted and absorbed by atoms.
Asymptotic giant Branch Star
Electromagnetic Radiation
Vernal Equinox
partile horizon
45. A push or a pull
force
Black Hole
Nebula
Steady State Theory (Leads to Olber's Paradox)
46. Poitns of gravitational stability in the orbit of a planet
Lagrangian Razor
Oort cloud
force
Hyashi track
47. A particle of light.
Primary Mirror
Brown dwarf
Photon
Instability strip
48. What is the universe expanding into?
Convection
Color Index
density parameter
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.
49. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Zenith
HII Region
Sc spiral galaxy
Magnification
50. Form honeycomb like patterns surrounding empty or nearly empty voids.
CNO Cycle
Absolute Magnitude
superclusters
Supernova (You can be my supernova girl)