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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 'edge' of the universe. Light beyond this has not reached us yet.
Turn off Point
mare basalt
partile horizon
radio galaxy
2. The dark - relativley smooth areas on the moon; Latin for sea
Black Hole
Precession
Maria
conjunction
3. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
CNO Cycle
Population 1 vs Population 2 stars
Enke gap
roche limit
4. When the Moon entirely blocks the Sun.
Atomic Number
Electromagnetic Radiation
Disk
Total Eclipse
5. 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
Absorption Spectrum
resonance
Dark matter candidates
6. The process responsible for creating the arms of flocculent spiral galaxies
Self-Propogating Star Formation
Total Eclipse
Photosphere
Supernova (You can be my supernova girl)
7. The name for the only seriously considered theory of the universe.
Void
Big Bang
shape and color of ELLIPTICAL galaxies
Make up of the terrestrial planets
8. Is space infinitely large?
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9. A change in the appearance of the sun at the edge of the solar disk
Halo
Spectroscopic Parallax
Energy Level
Limb darkening
10. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Ganymede (Jupiter)
force
Differential Rotation
blazar
11. The oldest part of the Milky Way
radiant
Halo
Dark Nebula
Synchrotron Rotation
12. A subatomic particle with a negative charge. It creates light.
Electron
Eclipses of the Moons of Jupiter
Planck time
AGN
13. Dying small mass stars lose their outer layers in a relatively gentle way - creating a round or bipolar nebula about the star (round like planets)
Particle Horizon
Geocentric
planetary nebula
meteoriod
14. A perfect absorber and radiator of electromagnetic radiation.
Electromagnetic Radiation: Infrared
CNO Cycle
Blackbody
supernova
15. 10^2 nm 10^7 nm
Electromagnetic Radiation: Gamma Ray
difference between maria and highlands of the moon.
differential rotation
semimajor axis
16. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
great red spot
Absolute Magnitude
Thermonuclear Fusion
Void
17. Large nebula consisting of very cold gas and dust
Occam's razor
dark energy
Molecular Clouds
Electromagnetic Radiation
18. The wavelengths where a specific element can absorb or emit light.
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
reflection star clusters
semimajor axis
Spectral Lines
19. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Europa (Jupiters moon)
Radio Galaxy
Kirkwood gaps
The Local Group
20. A very dense - highly populated cluster of galaxies
Electron
Chandrasekhar Limit
Rich Cluster
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.
21. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
general star population
AGN
Geocentric
Sunspot cycle
22. 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.
partile horizon
Magnification
era of recombination
differential rotation
23. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
The Local Group
Cosmic Microwave Background (CMB)
radiation dominated universe
dark energy
24. A logarithmically scaled value for the measured brightness of a star.
Perihelion
Ionization
Apparent Magnitude
synchronous rotation
25. The material from which the solar system formed
meteor
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.
solar nebula
gravity
26. Electromagnetic Radiation
Cosmic Microwave Background (CMB)
Supercluster
Planck time
A family of radiant energy- includes light
27. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
chemical differentiation
Corona
CCD
28. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Light Gathering Power
Thickest atmosphere
Plague
Focal Length
29. The larger bodies that formed early in teh solar nebula that were chemically differentiated
Io (jupiters moon)
Metals
Umbra
planetesimal
30. The average distance between the Earth and the Sun (=1.5 x10^8km)
resonance
quasar
Astronomical Unit
Refractor
31. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
A family of radiant energy- includes light
Europa (Jupiters moon)
partile horizon
cosmological principle
32. 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.
Primary Mirror
CMB
Nebula
Dwarf planets
33. Highlands: rocks are made of lighter anorthosite (similar to old earth rocks) Maria: rocks made of heavy mare basalt (volcanic rock) everywhere else is loose regolith created by meteoric impact.
Negative - Diverge - Less than 1
Planck time
difference between maria and highlands of the moon.
standard candle
34. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
Flocculent spirals
mass
Total Eclipse
Negative - Diverge - Less than 1
35. The area behind a lens where images are resolved
Apparent Magnitude
Focal Plane
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
meteoriod
36. When the Sun moves from south to north across the celestial equator (about March 21)
greatest elongation
Halo
Vernal Equinox
Plank's Law
37. The temp at which a substance in the vacuum of space solidifies
MOONS: roundest shape
Bulge
Dark Matter
condensation temperature
38. The elementary building blocks from which protons and neutrons are formed.
Wein's Law
Bulge
The Big Bang Theory
quarks
39. Moon in less than the angular diameter of the Sun.
Synodic Day
Rich Cluster
Annular Eclipse
Molecular Clouds
40. The elementary building blocks from which protons and neutrons are formed.
Sb spiral galaxy
quarks
Color Index
Disk
41. An important quality of telescopes that increases as the square of the primary mirror or objective lens
quasar
solar nebula
cosmic fireball
Light Gathering Power
42. Collections of young - hot stars
Shepherd satellite
OB Associations
Kuiper belt
Spectral Lines
43. Small compact stars called white dwarfs can have material deposited on their surfaces. In time material heats up and explodes in surface nuclear reaction- star brightens - settles - repeats.
Celestial Equator
Kuiper belt
nova
roche limit
44. How is the Hubble Law consistent with an expanding universe?
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.
Planck time
Seyfert galaxy
mass
45. The dimming of starlight by intervening dust
Cepheid variables
Interstellar Extinction
Perihelion
Red Giant Branch Star
46. The class of all objects having high energy radiation coming from their nuclei. Active Galactic Nucleus- Blazars - Quasars - Radio and Emit synchrotron radiation
rotation curve = dark matter?
MOONS: roundest shape
AGN
Electromagnetic Radiation: X-Ray
47. The location in the Milky Way where stars orbit like a solid wheel
Convection
Bulge
Reflector
nucleus
48. First accurately measured the speed of light in a vacuum
Nova
Ole Roemer
great dark spots
Ganymede (Jupiter)
49. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
accretion disk
Make up of the terrestrial planets
Nebula
Sa spiral galaxy
50. Jupiter
Negative - Diverge - Less than 1
fastest rotation
planetesimal
We don't know. It might be but does not have to be.