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Test your basic knowledge |
Cosmology
Start Test
Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
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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. When the Sun moves from south to north across the celestial equator (about March 21)
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
reflection star clusters
general star population
Vernal Equinox
2. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Black Hole
most moons
rotation curve = dark matter?
The Local Group
3. Jupiter
fastest rotation
Electromagnetic Radiation: X-Ray
shape and color of SPIRAL galaxies
Electromagnetic Radiation: Radio
4. When a planet lines up with the sun inthe sky
critical density
conjunction
Coldest surface
Hydrostatic Equilibrium
5. 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.
shape and color of SPIRAL galaxies
era of recombination
standard candle
quasar
6. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
meteor
Titus-Bode Law
roche limit
density waves
7. N=are*Fp(Ne)(Fl)(Fi)(Fc)(L) N: number of civilizations possible to communicate with are*: rate solar-like stars are created Fp: fraction of stars with planets Ne: number of planets like ours Fl: fraction of planets with life Fi: intelligent life Fc:
H2 Regions
Titus-Bode Law
Objective Lens
Drake equation
8. The apparent backward motion of a planet against the background of stars.
Main Sequence Stars
retrograde motion
MOONS: larger than mercury
Europa (Jupiters moon)
9. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Open - flat - and closed.
CNO Cycle
Prominence
dark matter
10. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Active Optics
most moons
blazar
rotation curve=winding dilemma?
11. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
Jupiters red spot
Quasar
direct motion
Asymptotic giant Branch Star
12. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
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.
Molecular Clouds
Rich vs poor clusters
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.
13. Orbit in Jupiters orbit
Proton-proton chain
Gamma-ray Burst
Trojan asteroids
Density Wave
14. Light-colored high-pressure bands in Jupiter's atmosphere
Electromagnetic Radiation
belt
fusion crust
zone
15. A collection of galaxies like the one the Milky Way belongs to
Poor Cluster
Supernova (You can be my supernova girl)
Callisto (Jupiter)
Gamma-ray Burst
16. Radiation given off by electrons accelerating in a magnetic field
Synchrotron Rotation
partile horizon
semimajor axis
Rich Cluster
17. A location on an H-are Diagram where evolving stars pulsate
Proton-proton chain
radio lobe
Total Eclipse
Instability strip
18. Extends to a distance of 50000AU. Same objects as in the Kuiper belt-when they fall in toward the sun they become comets. Debris from comets hitting the Earths atmosphere cause meteor showers.
Oort Cloud
Dark matter candidates
Dark Nebula
Callisto (Jupiter)
19. A high-pressure bulge in Neptune's southern hemisphere
Synodic Day
great dark spots
Pulsar
least dense
20. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
Hyashi track
Apparent Magnitude
Void
radio galaxy
21. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Planck time
anorthosite
rotation curve=winding dilemma?
Parsec
22. A phenomenon seen when the Earth passes through the orbit of a burned out comet
density
meteor shower
MOONS: larger than mercury
Gamma ray bursts
23. Light scattered through the atmosphere that degrades astronomical images
Light-Year
H-are Diagram
Light Pollution
Reflector
24. Any class of objects with a uniform luminosity used to determine distance.
standard candle
radiation pressure
Magnification
Flat - Flat
25. A push or a pull
force
opposition
Kuiper belt
rotation curve=winding dilemma?
26. A representation of the changes in color and brightness of an evolving protostar.
Yes - frozen at the poles- remains protected from the suns rays
condensation temperature
Hyashi track
meteorite
27. 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.
Most dense
Absorption Spectrum
superclusters
mapping the structure of Milky Way disk
28. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Light Gathering Power
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.
Cosmic Microwave Background
Light-Year
29. A star that erratically and explosively brightens and dims
Nova
Neutron Star
anorthosite
White Dwarf
30. The oldest terrain on the moon
great dark spots
highlands
Chromosphere
Nebula
31. A small chunk of rock in space
chondrite
meteoriod
Resolving Power
dark matter
32. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Photometry
Brown dwarf
Horizontal Branch Star
Maria
33. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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34. A distance measure determined by the shifting of a star against the background sky every 6 months.
protostar
Blackbody Curve
Neutron Star
Parsec
35. That which is responsible for Jupiter's magnetic field
coma
Liquid metallic hydrogen
Thermal Equilibrium
Self-Propogating Star Formation
36. In a FLAT UNIVERSE(our universe) - the curvature of space-time is ________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
evidence of water on mars
Flat - Remain Parallel - Exactly 1
conjunction
Vernal Equinox
37. A galaxy sending out a stream of material from its nucleus
CCD
Granules
Radio Galaxy
Absorption Spectrum
38. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
Rich Cluster
gravity
We don't know. It might be but does not have to be.
asteroid
39. The light produced when particles from the sun collide with atmospheric molecules
aurora
chondrite
slowest rotation
CCD
40. The process that powers the sun and hydrogen bombs
Positive - Converge - Greater than 1
Thermonuclear Fusion
rotation curve=winding dilemma?
Big Bang
41. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
Kuiper belt
self-propagating star formation
Light Pollution
Flat - Flat
42. A continuous spectrum of light missing energy at a few wave lengths.
Absorption Spectrum
quarks
difference between maria and highlands of the moon.
Lagrangian Razor
43. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
tectonics of Earth
difference between maria and highlands of the moon.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Reflector
44. The lens that gathers the light in a refractor
Objective Lens
Flocculent spirals
SETI
Self-Propogating Star Formation
45. What is the universe expanding into?
Chromosphere
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.
E=mc2
anorthosite
46. 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)
Filament
Planck time
molecular clouds
Bok Globule
47. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Radio Galaxy
Convection
Sa spiral galaxy
fusion crust
48. The Big Bang was not an explosion of matter into empty space - like the explosion of a bomb. Instead - it was an emergence of space and time filled with pure energy where before none of this was present. The point from which is emerged is called the
cosmological principle
The Big Bang Theory
300000 KM/sec
dark matter
49. The shadow area behind the Earth or Moon where the Sun is completely obscured.
terrestrial planet
Sc spiral galaxy
contrast northern lowlands and the southern highlands of mars...
Umbra
50. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
Sunspot cycle
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
supernova
cosmic fireball
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