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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. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
radiation dominated universe
meteor shower
The Big Bang Theory resolves Olber's Paradox
synchrotron radiation
2. How is the Hubble Law consistent with an expanding universe?
Celestial Sphere
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.
Kirchhoff's Law
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.
3. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
Big Crunch
Hubble law
Magnification
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.
4. A galaxy sending out a stream of material from its nucleus
inferior planets
Milky way Galaxy
shape and color of ELLIPTICAL galaxies
Radio Galaxy
5. Infinitely long -> 10 cm
Electromagnetic Radiation: Radio
roche limit
Most dense
Turn off Point
6. The rotation period of the Earth measured relative to the stars.
Sidereal Day
protostar
Light Curve
Halo
7. A faint - remarkably uniform distribution of radiation in space
Steady State Theory (Leads to Olber's Paradox)
OB Associations
synchronous rotation
Cosmic Microwave Background
8. A term referring to the orbital character of stars near the Sun
Cosmic Microwave Background
quasar
Differential Rotation
Focal Plane
9. A bridge of material held in position above the solar surface. They can remain for hours even days
Interstellar Extinction
Prominence
CCD
chemical differentiation
10. When the Sun is farthest south of the celestial equator (About December 22)
Winter Solstice
supermassive black hole
Jovian Planets
Light Pollution
11. A very dense - highly populated cluster of galaxies
Rich Cluster
cosmological principle
Kuiper belt
Interstellar Extinction
12. In what chemical form are jupiters nitrogen - carbon and oxygen?
Light-Year
Ammonia - methane - and water
Kuiper belt
Eclipses of the Moons of Jupiter
13. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
resonance
coma
Kuiper belt
Sa spiral galaxy
14. Long - meandering cliff formed when a planet surface cools and shrinks
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.
Gamma ray bursts
Parsec
scarp
15. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Chromosphere
critical density
Reflector
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.
16. When particles are compressed to an unnatural state where their pressure is not related to their temperature
Gamma-ray Burst
Make up of the jovian planets
Degeneracy
Europa (Jupiters moon)
17. A star without enough mass to begin hydrogen fusion
Heliocentric
Spectroscopic Parallax
Brown dwarf
Resolving Power
18. The 'edge' of the universe. Light beyond this has not reached us yet.
Thermal Equilibrium
Plank's Law
Flat - Flat
partile horizon
19. 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
Positive - Converge - Greater than 1
SETI
disk
Thermonuclear Fusion
20. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
radio galaxy
density
shape and color of SPIRAL galaxies
Open Cluster
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.
Self-Propogating Star Formation
H2 Regions
evidence of water on mars
mapping the structure of Milky Way disk
22. An entity that is likely in the nucleus of most - if not all - galaxies.
HII Region
supermassive black hole
fusion crust
Open Cluster
23. The surface of the sun
Winter Solstice
Photosphere
Kirchhoff's Law
Magnification
24. The mix of pure photon energy that emerged at the start of the universe.
cosmic fireball
planetary nebula
Particle Horizon
Most dense
25. A bright area of higher temperature that often proceeds the formation of sunspots.
MOONS: thickest atmosphere
Absolute Magnitude
Ionization
Plague
26. Moon in less than the angular diameter of the Sun.
Population 1 vs Population 2 stars
AGN
Annular Eclipse
Active Optics
27. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Kirkwood gaps
Wein's Law
great dark spots
Red Giant
28. 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
If it is in a denser medium - such as glass - it will move slower
Open Cluster
most eccentric orbit
29. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Neutron Star
mass
radiation dominated universe
Seyfert galaxy
30. After stars form they pump light energy into surrounding gas causing it to heat up and glow (H2=ionized hydrogen - H1= neutral hydrogen in molcular couds)
H2 Regions
Spectroscopy
most moons
Yes - frozen at the poles- remains protected from the suns rays
31. 1-orbit aroudn the sun 2- are in hydrostatic equilibrium and 'mostly round' 3- have not cleared debris around its orbit 4- are not satellites
cosmology
Dwarf planets
Titus-Bode Law
Disk
32. The location in the Milky Way where stars orbit like a solid wheel
Eyepiece Lens
Globular Cluster
Autumnal Equinox
Bulge
33. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Electromagnetic Radiation: X-Ray
jovian
Sb spiral galaxy
comet
34. Matter so dense that even light cannot escape its gravity
Black Hole
Gamma-ray Burst
Eclipses of the Moons of Jupiter
Light: travels like a wave - detected like a particle
35. When massive objects bend space and time enough to create multiple images of an object located behind them
direct motion
Gravitational Lens
Plague
radiation dominated universe
36. Is space infinitely large?
37. A planet that is farther from the sun than the Earth is
Superior planets
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.
Jupiters red spot
H2 Regions
38. 1 mm 1μm
Resolving Power
isotropic
Callisto (Jupiter)
Electromagnetic Radiation: Infrared
39. 10 nm 10^2 nm
Inverse Square Law
Electromagnetic Radiation: X-Ray
Apparent Magnitude
meteor shower
40. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
Void
Terrestrial Planets
Magnification
epicycle
41. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Sb spiral galaxy
Absorption Spectrum
Refractor
Asymptotic giant Branch Star
42. A planet that is farther from the sun than the Earth is
Neutron Star
MOONS: thickest atmosphere
Superior planets
belt
43. The mirror that gathers the light in a reflector
Primary Mirror
Globular 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
Instability strip
44. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Differential Rotation
Neutron Star
Make up of the terrestrial planets
belt
45. 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
The Big Bang Theory
Extrasolar Planet
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
plate tectonics
46. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
highlands
Supercluster
greehouse effects
47. A crystalline patter found in iron meteorites
Doppler Shift
Yes - frozen at the poles- remains protected from the suns rays
widmanstatten pattern
Electromagnetic Radiation: Radio
48. Approximate speed of light in a vacuum
300000 KM/sec
CNO Cycle
greehouse effects
most moons
49. A huge sphere of tenuous gas surrounding the nucleus of a comet
Filament
HII Region
Positive - Converge - Greater than 1
coma
50. Small moons that maintain the shape of rings around Saturn and Uranus
meteoriod
Negative - Diverge - Less than 1
Annular Eclipse
Shepherd satellite