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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.
partile horizon
aphelion
Prominence
Halo
2. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
meteorite
Asymptotic giant Branch Star
rotation curve=winding dilemma?
Ganymede (Jupiter)
3. The process that powers the sun and hydrogen bombs
Penumbra
Thermonuclear Fusion
coma
CMB
4. A collection of galaxies like the one the Milky Way belongs to
Rich Cluster
slowest rotation
Zenith
Poor Cluster
5. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
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6. The lowest energy of an atom.
Disk
Light Pollution
Ground State
quasar
7. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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8. The location in an H-are diagram of a star cluster - where stars have just left the main sequence. Used to estimate the cluster age.
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.
Turn off Point
resonance
mare basalt
9. A star that is in the process of forming. It glows from gravitational contraction
neutrino
protostar
Pixel
tectonics of Venus
10. Half of the longest diameter across an ellipse
semimajor axis
synchronous rotation
Interstellar Extinction
Refractor
11. 1μm 100 nm
Electromagnetic Radiation: Visible Light
differential rotation
Halo
most moons
12. A volume of space where few - if any - galaxies are located
Void
Ground State
The Big Bang Theory resolves Olber's Paradox
Ecliptic
13. The projection of the Earth's equator onto the celestial sphere.
accretion disk
homogeneous
Autumnal Equinox
Celestial Equator
14. A bridge of material held in position above the solar surface. They can remain for hours even days
Prominence
Zenith
condensation temperature
Light Gathering Power
15. Saturn
highlands
Plank's Law
least dense
accretion disk
16. A spinning neutron star
Pulsar
supernova
regolith
Black Hole
17. Centered on the sun.
Continuous Spectrum
synchronous rotation
Heliocentric
MOONS: roundest shape
18. When the Sun is farthest south of the celestial equator (About December 22)
Spectroscopic parallax
Winter Solstice
Gamma-ray Burst
dark matter
19. The seasonal shifting of a nearby star's position relative to more distant objects.
HII Region
Parallax
Magnification
Superior planets
20. A long-lived high-pressure bulge in Jupiter's southern hemisphere
3 reasons we orbit satellites to observe universe
Extrasolar Planet
great red spot
matter dominated universe
21. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
Convection
density parameter
reflection star clusters
Largest diameter
22. The mass of an object divided by its volume
Meridian
Photometry
Black Hole
density
23. Dark areas on the sun that are cooler than the surrounding photosphere
Sunspots
plate tectonics
self-propagating star formation
tectonics of Mars
24. When massive objects bend space and time enough to create multiple images of an object located behind them
Pixel
bulge
widmanstatten pattern
Gravitational Lens
25. A galaxy emitting large amounts of energy at long wavelengths.
Blackbody
Hydrostatic Equilibrium
radio galaxy
Electromagnetic Radiation: Radio
26. A younger cluster of stars - found in the galaxy disk
Open Cluster
Make up of the terrestrial planets
Triple Alpha rocess
Emission Spectrum
27. The family of radiant energy that includes light as a subset
deferent
planetary nebula
Electromagnetic Radiation
fusion crust
28. Finding a star's absolute magnitude from it's placement on an HR diagram. After finding the absolute magnitude - we measure the apparent magnitude - for a distance modulus and use this to find the distance. This method is good for finding distances t
smallest diameter
Atomic Number
Spectroscopic parallax
superclusters
29. A spread of light with an uninterrupted wavelength distribution of energy.
Continuous Spectrum
homogeneous
anorthosite
quarks
30. The entity from which the whole universe is postulated to have come from.
Hubble constant
Steady State Theory (Leads to Olber's Paradox)
Extrasolar Planet
cosmic singularity
31. Mercury and venus
Flat - Flat
Dark matter candidates
Electromagnetic Radiation: Microwave
fewest moons
32. The apparent path of the Sun through the stars on the celestial sphere.
H-are Diagram
contrast northern lowlands and the southern highlands of mars...
Ecliptic
semimajor axis
33. Earth
Most dense
Sb spiral galaxy
weight
density
34. 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)
Ganymede (Jupiter)
shape and color of ELLIPTICAL galaxies
H2 Regions
Sidereal Day
35. Hydrogen and helium (mainly)
Halo
era of recombination
Parallax
Make up of the jovian planets
36. A planet that is closer to the sun than the earth
meteorite
Colestial Pole
inferior planets
widmanstatten pattern
37. 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
Disk
Cosmic Microwave Background (CMB)
Electromagnetic Radiation: Infrared
38. Matter that reveals itself only through its gravitational attraction.
dark matter
direct motion
Yes - frozen at the poles- remains protected from the suns rays
Extrasolar Planet
39. The law that predicts the possible types of spectra.
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40. The larger bodies that formed early in teh solar nebula that were chemically differentiated
Coronal Loop
Flat - Flat
planetesimal
greehouse effects
41. An empirical scheme for predictin ghe orbital distances of planets
Titus-Bode Law
condensation temperature
Globular Cluster
Corona
42. A term referring to the orbital character of stars near the Sun
Pulsar
Light Curve
Differential Rotation
Europa (Jupiters moon)
43. A word meaning 'the same in all directions.'
Electromagnetic Radiation: Microwave
isotropic
Electromagnetic Radiation
radiation dominated universe
44. What are the three possible geometries of the universe?
nucleus
mass
Open - flat - and closed.
Chromosphere
45. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
aurora
3 reasons we orbit satellites to observe universe
cosmic fireball
quarks
46. A prominence seen against the disk of the sun
Filament
Lagrangian Razor
E=mc2
Yes - frozen at the poles- remains protected from the suns rays
47. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
Galilean satellite
Perihelion
Io (jupiters moon)
shape and color of ELLIPTICAL galaxies
48. A push or a pull
force
Synodic Day
Sunspot cycle
Radiative Diffusion
49. A change in the wavelength of light caused by a motion between the observer and light (or wave) source (blue shift if getting closer - red shift if moving away)
meteoriod
Doppler Shift
meteor shower
belt
50. The part of the Milky way that has on-going star formation
Planetary Nebula
Disk
Degeneracy
terrestrial planet