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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 measure of the ability of a telescope to see fine detail
chemical differentiation
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
Resolving Power
Halo
2. Mercury
superclusters
smallest diameter
Quasar
Black Hole
3. The family of radiant energy that includes light as a subset
Focal Plane
Electromagnetic Radiation
Colestial Pole
The Big Bang Theory resolves Olber's Paradox
4. Approximate speed of light in a vacuum
300000 KM/sec
Make up of the terrestrial planets
weight
Dark Matter
5. The fusion process that turns three helium nuclei into a carbon nucleus
Triple Alpha rocess
Red Giant
Differential Rotation
shape and color of SPIRAL galaxies
6. Any change in the speed or direction of an object's motion
Coronal Loop
Largest diameter
Shepherd satellite
acceleration
7. An entity that is likely in the nucleus of most - if not all - galaxies.
neutrino
Make up of the terrestrial planets
Objective Lens
supermassive black hole
8. 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 Venus
conjunction
Kuiper belt
tectonics of Mars
9. Population 1- similar to the sun and 2% of elements are metal - Population 2- formed before gas was metal- only a fraction of mass is metal.
Umbra
Population 1 vs Population 2 stars
Electromagnetic Radiation: X-Ray
Thickest atmosphere
10. An energetic event taking place in the early universe
inferior planets
Cepheid variables
fusion crust
Gamma-ray Burst
11. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
hottest surface
protostar
Negative - Diverge - Less than 1
Brown dwarf
12. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Ganymede (Jupiter)
Electromagnetic Radiation: Visible Light
Winter Solstice
Apollo asteroids
13. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
The Local Group
Positive - Converge - Greater than 1
resonance
E=mc2
14. What causes the zones and belts on jupiter and saturn?
dark matter
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
300000 KM/sec
Interstellar Extinction
15. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
synchronous rotation
Big Crunch
Light-Year
Gamma ray bursts
16. The normal eastward movement of a planet against the background of hte distant stars.
self-propagating star formation
direct motion
Big Crunch
blazar
17. How is the Hubble Law consistent with an expanding universe?
Horizontal Branch Star
matter dominated 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.
anorthosite
18. The cosmological principle is the assumption that the universe is isotropic and homogeneous.The Big Bang assumes it to be a correct principle so that what we observe is exactly like What is too far away to be observed.
accretion
shape and color of SPIRAL galaxies
Electromagnetic Radiation: Visible Light
Cosmological Principle
19. The point in its orbit where a planet is farthest from the sun
aphelion
cosmology
cosmic singularity
Roundest orbit
20. 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)
homogeneous
MOONS: most geologically active
Electron
planetary nebula
21. Matter that reveals itself only through its gravitational attraction
Dark Matter
meteorite
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.
Oort Cloud
22. A perfect absorber and radiator of electromagnetic radiation.
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.
rotation curve=winding dilemma?
Blackbody
Convection
23. An empirical scheme for predictin ghe orbital distances of planets
cosmic fireball
Titus-Bode Law
Electromagnetic Radiation: Ultraviolet Light
Planetary Nebula
24. 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...
widmanstatten pattern
300000 KM/sec
Supernova (You can be my supernova girl)
25. A star that erratically and explosively brightens and dims
Light Gathering Power
condensation temperature
fastest rotation
Nova
26. Mercury
thinnest atmosphere
Coldest surface
critical density
most eccentric orbit
27. A faint - remarkably uniform distribution of radiation in space
Cosmic Microwave Background
Big Crunch
Instability strip
Horizontal Branch Star
28. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Light: travels like a wave - detected like a particle
Zenith
Self-Propogating Star Formation
The Local Group
29. IO
highlands
MOONS: most geologically active
Energy Level
belt
30. The movement of the Earth's crustal plates riding on top of the mantle.
quasar
most moons
Sc spiral galaxy
plate tectonics
31. 10 cm -> 1 mm
Primary Mirror
Plague
Electromagnetic Radiation: Microwave
Electromagnetic Radiation: Infrared
32. Jupiter
fastest rotation
Kirchhoff's Law
Vernal Equinox
great dark spots
33. Centered on the Earth
Flat - Remain Parallel - Exactly 1
Geocentric
slowest rotation
supermassive black hole
34. A bright area of higher temperature that often proceeds the formation of sunspots.
epicycle
Neutron Star
Plague
cosmic singularity
35. A term referring to the orbital character of stars near the Sun
Open - flat - and closed.
radio lobe
homogeneous
Differential Rotation
36. A prominence seen against the disk of the sun
Sc spiral galaxy
Filament
meteor shower
Ionization
37. A long-lived high-pressure bulge in Jupiter's southern hemisphere
great red spot
Cepheid variables
Photosphere
Rich vs poor clusters
38. The rate of expansion of the universe.
Hydrostatic Equilibrium
rotation curve = dark matter?
Radio Galaxy
Hubble constant
39. A telescope that uses lenses to focus light
Secondary Mirror
radiation pressure
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
Refractor
40. That which is responsible for Jupiter's magnetic field
Bulge
Ionization
Liquid metallic hydrogen
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.
41. IO
self-propagating star formation
The Local Group
MOONS: most geologically active
Seyfert galaxy
42. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Supernova (You can be my supernova girl)
Light-Year
If it is in a denser medium - such as glass - it will move slower
zone
43. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
density waves
Extrasolar Planet
least dense
CCD
44. Hydrogen and helium (mainly)
Cepheid variables
cosmic singularity
Electromagnetic Radiation: X-Ray
Make up of the jovian planets
45. 1. We see rapid movements or high energy radiation coming at some level from the nuclei of nearly every galaxy we have looked at. 2. We suspect that the creation of these supermassive black holes is part of the galaxy formation process.
Jovian Planets
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
supernova
direct motion
46. When material is heated and moves taking the heat energy with it
Heliocentric
Convection
radiation pressure
Parallax
47. The measure of a variable star's apparent magnitude as it brightens and dims with time
Light Curve
meteoriod
partile horizon
supernova
48. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
CNO Cycle
Resolving Power
A family of radiant energy- includes light
Nebula
49. 1. We see rapid movements or high energy radiation coming at some level from the nuclei of nearly every galaxy we have looked at. 2. We suspect that the creation of these supermassive black holes is part of the galaxy formation process.
Spectroscopic Parallax
Supercluster
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Energy Level
50. The number of protons in an atom.
Limb darkening
cosmological red shift
Atomic Number
Emission Spectrum