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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. 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.
meteorite
CMB
Oort Cloud
Stephen-Boltzman Law
2. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
Parallax
Cosmic Microwave Background
force
deferent
3. Why does the earth have few craters while the moon has many?
Eyepiece Lens
Supercluster
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
cosmic singularity
4. Collections of young - hot stars
Astronomical Unit
OB Associations
shape and color of ELLIPTICAL galaxies
era of recombination
5. The law that syas light energy from a blackbody increases as (temperature^4)
Stephen-Boltzman Law
Vernal Equinox
Precession
Resolving Power
6. The point in its orbit where a planet is nearest the sun
Disk
Gamma-ray Burst
deferent
Perihelion
7. VENUS
Ganymede (Jupiter)
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
Globular Cluster
Light Gathering Power
8. A spectrum of light with energy at only a few wavelengths.
Blackbody Curve
Emission Spectrum
most eccentric orbit
Spectroscopic Parallax
9. That which is responsible for Jupiter's magnetic field
Granules
radio galaxy
solar nebula
Liquid metallic hydrogen
10. The rotation period of the Earth measured relative to the Sun.
Superior planets
Synodic Day
Metals
Blackbody Curve
11. Jupiter
quarks
fastest rotation
Hubble constant
epicycle
12. Saturn
Density Wave
least dense
MOONS: larger than mercury
Perihelion
13. A star that is burning hydrogen to helium in a shell surrounding it's core
Roundest orbit
Heliocentric
Red Giant Branch Star
Active Optics
14. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
self-propagating star formation
Coldest surface
Dark Nebula
Focal Plane
15. A streak of light in the atmosphere
Electromagnetic Radiation: Gamma Ray
meteor
Brown dwarf
Thermonuclear Fusion
16. A measure of the seasonal shifting of a star's position against farther stars or galaxies. The closer the star - the greater is the angular distance it shifts. We use it to find distances to stars that are up to 1000 pc away.
Spectroscopic Parallax
Parallax
semimajor axis
direct motion
17. In what chemical form are jupiters nitrogen - carbon and oxygen?
Ground State
radio galaxy
chondrite
Ammonia - methane - and water
18. Poitns of gravitational stability in the orbit of a planet
Flat - Remain Parallel - Exactly 1
aurora
Photon
Lagrangian Razor
19. As open clusters age - they push gas away but dust remains this can reflect light giving the cluster a blue-ish color. also called reflection nebula
critical density
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.
reflection star clusters
planetesimal
20. A star that blows itself apart
regolith
MOONS: thickest atmosphere
Supernova (You can be my supernova girl)
Superior planets
21. The larger bodies that formed early in teh solar nebula that were chemically differentiated
planetesimal
plate tectonics
radiation pressure
Make up of the terrestrial planets
22. We can infer the absolute magnitude of pulsating variable stars by measuring their pulsation periods. The longer the pulsations - the greater their luminosities. We then again measure their apparent magnitudes - compare it with their absolute magnitu
Umbra
Cepheid variables
regolith
matter dominated universe
23. Young clusters in disk are irregularly shaped since they have no time to relax into the rounder relaxed shape of globular clusters-will constantly be torn apart and assimilated.
Turn off Point
Flat - Flat
Globular Cluster
open star clusters
24. Radiation given off by electrons accelerating in a magnetic field
Callisto (Jupiter)
Synchrotron Rotation
anorthosite
Dark Matter
25. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Interstellar Extinction
If it is in a denser medium - such as glass - it will move slower
direct motion
zone
26. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
quarks
opposition
Yes - frozen at the poles- remains protected from the suns rays
CNO Cycle
27. 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
force
hottest surface
Meridian
28. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
H-are Diagram
Neutron Star
fewest moons
general star population
29. 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
High Velocity Stars
AGN
radiation pressure
30. The material from which the solar system formed
solar nebula
force
Eclipses of the Moons of Jupiter
Electromagnetic Radiation: Infrared
31. A force exerted by reflecting sunlight
Most dense
radiation pressure
Cepheid variables
Winter Solstice
32. A term referring to the orbital character of stars near the Sun
Globular Cluster
condensation temperature
Differential Rotation
accretion
33. A very dense - highly populated cluster of galaxies
radio galaxy
H-are Diagram
Light Pollution
Rich Cluster
34. The sinking of denser elements to the center of a young molten planet
Make up of the terrestrial planets
supermassive black hole
chemical differentiation
quarks
35. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Secondary Mirror
The Local Group
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
differential rotation
36. Hydrogen and helium (mainly)
Make up of the jovian planets
Instability strip
Light: travels like a wave - detected like a particle
Cosmic Microwave Background (CMB)
37. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
Electromagnetic Radiation: Ultraviolet Light
Roundest orbit
Rich vs poor clusters
condensation temperature
38. The high- temperatature outer layer of the sun
H2 Regions
Corona
asteroid
Astronomical Unit
39. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
Sunspot cycle
300000 KM/sec
molecular clouds
Rich Cluster
40. Matter that reveals itself only through its gravitational attraction.
meteorite
Parallax
Planck time
dark matter
41. A spread of light with an uninterrupted wavelength distribution of energy.
Continuous Spectrum
Red Giant
Main Sequence
era of recombination
42. A telescope that uses lenses to focus light
Chromosphere
partile horizon
Refractor
reflection star clusters
43. When the Sun is farthest south of the celestial equator (About December 22)
Winter Solstice
Summer Solstice
MOONS: largest size
retrograde motion
44. A force exerted by reflecting sunlight
Neutron Star
shape and color of ELLIPTICAL galaxies
radiation pressure
zone
45. The gap etween saturn's A and B rings
Positive - Converge - Greater than 1
Eyepiece Lens
Cassini division
CNO Cycle
46. We can infer the absolute magnitude of pulsating variable stars by measuring their pulsation periods. The longer the pulsations - the greater their luminosities. We then again measure their apparent magnitudes - compare it with their absolute magnitu
chemical differentiation
Main Sequence
Cepheid variables
Kuiper belt
47. The apparent path of the Sun through the stars on the celestial sphere.
cosmic fireball
Ecliptic
Shepherd satellite
Penumbra
48. The rock that makes up the lunar maria
mare basalt
great red spot
Bok Globule
Make up of the jovian planets
49. Mercury and venus
Wein's Law
fewest moons
Electromagnetic Radiation: Visible Light
critical density
50. The faint glow of light left over from the Big Bang. cosmic microwave background are the photons that remain after the big bang that have not turned into matter.
Nebula
Ganymede (Jupiter)
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
CMB