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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 source of the force that is accelerating the expansion rate of the universe.
Ionization
dark energy
superclusters
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
2. Star speed at outer edge of galaxy should begin to diminish - but they dont so we guess that this means there is increasing force (aka dark matter)
We don't know. It might be but does not have to be.
Emission Spectrum
condensation temperature
rotation curve = dark matter?
3. A very dense - highly populated cluster of galaxies
supermassive black hole
Rich Cluster
Kirkwood gaps
rotation curve = dark matter?
4. Collections of young - hot stars
accretion
Ground State
Energy Level
OB Associations
5. In what chemical form are jupiters nitrogen - carbon and oxygen?
Chandrasekhar Limit
Focal Plane
Ammonia - methane - and water
cosmic fireball
6. The process responsible for creating the arms of flocculent spiral galaxies
Parsec
Self-Propogating Star Formation
Terrestrial Planets
quarks
7. 10 nm 10^2 nm
Neutron Star
Cassegrain Focus
most eccentric orbit
Electromagnetic Radiation: X-Ray
8. A planet orbiting about a distant star
The Local Group
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
Extrasolar Planet
Kirchhoff's Law
9. A term referring to Jupiter-like planets
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.
Gamma-ray Burst
Cosmic Microwave Background (CMB)
jovian
10. Material that shoots rapidly out into space. Flares cause Auroras
rotation curve = dark matter?
Flare
Objective Lens
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
11. 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
Thermonuclear Fusion
Planetary Nebula
bulge
Synodic Day
12. The entity from which the whole universe is postulated to have come from.
Dark matter candidates
quasar
cosmic singularity
tectonics of Earth
13. A streak of light in the atmosphere
Ammonia - methane - and water
meteor
Ole Roemer
Active Optics
14. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
Most dense
evidence of water on mars
Electromagnetic Radiation: Infrared
Rich vs poor clusters
15. A quantity measuring the stability of the Earth's atmosphere
tectonics of Venus
Thermonuclear Fusion
Seeing
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
16. A plot of star absolute magnitude verses spectral type.
H-are Diagram
Grand design spirals
semimajor axis
Poor Cluster
17. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
Electromagnetic Radiation: Radio
neutrino
Hydrostatic Equilibrium
Meridian
18. A phenomenon seen when the Earth passes through the orbit of a burned out comet
meteor shower
Electromagnetic Radiation
neutrino
Pixel
19. A word meaning 'the same everywhere throughout.'
Occam's razor
Drake equation
homogeneous
Spectral Lines
20. The average distance between the Earth and the Sun (=1.5 x10^8km)
Astronomical Unit
Black Hole
gravity
Meridian
21. Light-colored high-pressure bands in Jupiter's atmosphere
radiant
zone
Continuous Spectrum
Electromagnetic Radiation: X-Ray
22. When material is heated and moves taking the heat energy with it
Convection
Rich vs poor clusters
Pulsar
Color Index
23. The apparent path of the Sun through the stars on the celestial sphere.
dark matter
Ecliptic
Electromagnetic Radiation: Microwave
fusion crust
24. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
bulge
Halo
Corona
Kuiper belt
25. 1μm 100 nm
The Big Bang Theory resolves Olber's Paradox
Poor Cluster
Electromagnetic Radiation: Visible Light
Apollo asteroids
26. The place in the sky that the Earth's axis points toward (can be either north or south)
The Big Bang Theory resolves Olber's Paradox
Colestial Pole
Kuiper belt
slowest rotation
27. The number of protons in an atom.
Superior planets
retrograde motion
Atomic Number
greehouse effects
28. Loops that trace the magnetic field as it erupts from a sunspot area and arches over to an adjacent area. They glow in the light of gas pouring out of corona and falling into photosphere.
disk
Coronal Loop
critical density
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
29. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Blackbody
quasar
Nebula
Light Curve
30. When the Sun moves from south to north across the celestial equator (about March 21)
Vernal Equinox
neutrino
accretion disk
Meridian
31. The point in its orbit where a planet is nearest the sun
High Velocity Stars
Perihelion
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.
Largest diameter
32. What Ole Roemer used to measure the speed of light in a vacuum
Eclipses of the Moons of Jupiter
Hubble law
Particle Horizon
comet
33. The process of acquiring material
Roundest orbit
If it is in a denser medium - such as glass - it will move slower
Winter Solstice
accretion
34. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Dwarf planets
slowest rotation
Absorption Spectrum
3 reasons we orbit satellites to observe universe
35. Matter that reveals itself only through its gravitational attraction.
High Velocity Stars
dark matter
The Local Group
Focal Length
36. A spinning neutron star
Light Pollution
Rich Cluster
Pulsar
Photometry
37. A star without enough mass to begin hydrogen fusion
Apparent Magnitude
Synodic Day
chondrite
Brown dwarf
38. A high-pressure bulge in Neptune's southern hemisphere
great dark spots
Light-Year
Dwarf planets
Turn off Point
39. A star that is burning hydrogen to helium in a shell surrounding it's core
chemical differentiation
Thickest atmosphere
Red Giant Branch Star
thinnest atmosphere
40. IO
MOONS: most geologically active
Oort Cloud
Radio Galaxy
mapping the structure of Milky Way disk
41. 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.
Secondary Mirror
Autumnal Equinox
era of recombination
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.
42. Approximate speed of light in a vacuum
Positive - Converge - Greater than 1
Hyashi track
300000 KM/sec
Eyepiece Lens
43. The location around an atom where an electron resides.
Energy Level
Magnification
Proton-proton chain
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
44. The powdered stone fragments that make up the lunar 'soil'
Spectroscopic parallax
regolith
protostar
Molecular Clouds
45. The displacement of spectral lines to redder colors caused by the expansion of the universe.
Thermonuclear Fusion
cosmological red shift
thinnest atmosphere
Vernal Equinox
46. Centered on the Earth
Geocentric
Radio Galaxy
Radio Galaxy
Energy Level
47. 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.
mapping the structure of Milky Way disk
Sa spiral galaxy
Oort Cloud
plate tectonics
48. The organization of clusters of galaxies into sheets and strings
Hyashi track
Electron
CNO Cycle
Supercluster
49. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Light Gathering Power
MOONS: most geologically active
synchrotron radiation
Reflector
50. The amount an image is enlarged by a telescope
acceleration
Main Sequence
Magnification
partile horizon