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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 layer of the sun just above the photosphere
Make up of the jovian planets
Ecliptic
cosmology
Chromosphere
2. 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
Extrasolar Planet
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Hubble law
Cepheid variables
3. When one side of a body always faces the planet it revolves around
synchronous rotation
meteor shower
most moons
Light Pollution
4. Jupiter
cosmological principle
OB Associations
most moons
Superior planets
5. The name for the only seriously considered theory of the universe.
Big Bang
MOONS: larger than mercury
condensation temperature
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.
6. A star that blows itself apart
Summer Solstice
Supernova (You can be my supernova girl)
The Big Bang Theory
3 reasons we orbit satellites to observe universe
7. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
highlands
CCD
Sunspot cycle
epicycle
8. A bridge of material held in position above the solar surface. They can remain for hours even days
radio lobe
Prominence
cosmological principle
thinnest atmosphere
9. Any change in the speed or direction of an object's motion
plate tectonics
acceleration
Electromagnetic Radiation: X-Ray
Big Crunch
10. Venus (retrograde)
Molecular Clouds
fastest rotation
slowest rotation
Plank's Law
11. The rotation period of the Earth measured relative to the stars.
mare basalt
Ground State
H-are Diagram
Sidereal Day
12. Any class of objects with a uniform luminosity used to determine distance.
cosmic fireball
Prominence
radiant
standard candle
13. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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14. Hydrogen and helium (mainly)
isotropic
Make up of the jovian planets
density
Trojan asteroids
15. 100 nm 10 nm
Resolving Power
meteor
MOONS: thickest atmosphere
Electromagnetic Radiation: Ultraviolet Light
16. Mercury and venus
fewest moons
Bulge
Hydrostatic Equilibrium
coma
17. The average distance between the Earth and the Sun (=1.5 x10^8km)
Eyepiece Lens
Electron
Astronomical Unit
planetary nebula
18. The seasonal shifting of a nearby star's position relative to more distant objects.
Parallax
accretion disk
greehouse effects
Big Bang
19. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Supercluster
Flat - Flat
synchrotron radiation
Colestial Pole
20. Any class of objects with a uniform luminosity used to determine distance.
Triple Alpha rocess
Geocentric
standard candle
OB Associations
21. A small and dim but hot star.
widmanstatten pattern
White Dwarf
least dense
Molecular Clouds
22. Stars fromt he Halo that have drifted into the disk. as earth zooms past them in a faster orbit they appear to be going backward very fast
High Velocity Stars
MOONS: larger than mercury
Rich vs poor clusters
Absorption Spectrum
23. A massive variable star used to find distances to the galaxies or clusters that contain them.
most eccentric orbit
Cepheid Variable
acceleration
Drake equation
24. A spread of light with an uninterrupted wavelength distribution of energy.
Open - flat - and closed.
Flare
Energy Level
Continuous Spectrum
25. The dimming of starlight by intervening dust
Heliocentric
Ionization
Interstellar Extinction
Electromagnetic Radiation: Infrared
26. Where is the center of the expansion
Electromagnetic Radiation
Chandrasekhar Limit
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.
Chromosphere
27. Jupiter - Saturn - Uranus - Neptune
hottest surface
Jovian Planets
Callisto (Jupiter)
Seyfert galaxy
28. A particle of light
Inverse Square Law
Photon
anorthosite
Globular Cluster
29. Clouds of low density gas often found glowing faintly on either side of an AGN.
White Dwarf
Electromagnetic Radiation
Hubble law
radio lobe
30. The distance light travels in one year (=9.46x10^12km).
Open - flat - and closed.
Differential Rotation
Light-Year
shape and color of ELLIPTICAL galaxies
31. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
roche limit
shape and color of SPIRAL galaxies
Resolving Power
Quasar
32. What is the universe expanding into?
Self-Propogating Star Formation
Nova
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.
nucleus
33. A star fusing hydrogen to helium in it's core
Main Sequence Stars
Enke gap
Electromagnetic Radiation: Infrared
Hipparchus
34. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Callisto (Jupiter)
Spectroscopy
radio galaxy
cosmology
35. The oldest part of the Milky Way
Halo
direct motion
Stephen-Boltzman Law
Photon
36. A star that is in the process of forming. It glows from gravitational contraction
Drake equation
protostar
Focal Plane
scarp
37. The fusion process that turns three helium nuclei into a carbon nucleus
Triple Alpha rocess
Ecliptic
Olber's paradox
Coronal Loop
38. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
slowest rotation
Red Giant
Sb spiral galaxy
Gamma-ray Burst
39. A planet that is closer to the sun than the earth
Most dense
inferior planets
synchrotron radiation
Electromagnetic Radiation: Radio
40. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Seyfert galaxy
Continuous Spectrum
Gravitational Lens
deferent
41. Infinitely long -> 10 cm
Electromagnetic Radiation: Radio
regolith
Cosmic Microwave Background
Thermal Equilibrium
42. The rotation of a star or planet at different speeds at its equator and poles
differential rotation
interstellar dust
cosmology
supermassive black hole
43. A small spherical dark nebula
synchronous rotation
Bok Globule
Magnification
Meridian
44. The layer of the sun just above the photosphere
Chromosphere
Open - flat - and closed.
Most dense
Wein's Law
45. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Density Wave
Main Sequence Stars
Eclipses of the Moons of Jupiter
Neutron Star
46. 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.
High Velocity Stars
MOONS: most geologically active
Oort Cloud
planetesimal
47. The process responsible for creating the arms of flocculent spiral galaxies
AGN
Europa (Jupiters moon)
Self-Propogating Star Formation
disk
48. The rotation period of the Earth measured relative to the Sun.
Flat - Flat
Synodic Day
deferent
Sunspot cycle
49. The place in the sky that the Earth's axis points toward (can be either north or south)
density
Maria
Colestial Pole
scarp
50. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
density waves
homogeneous
The Big Bang Theory resolves Olber's Paradox
MOONS: thickest atmosphere