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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 surface of the sun
Photosphere
self-propagating star formation
Blackbody
Galilean satellite
2. Titan
MOONS: most geologically active
MOONS: thickest atmosphere
Atomic Number
Thermal Equilibrium
3. 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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4. Jupiter
most moons
Secondary Mirror
Light-Year
nova
5. Light scattered through the atmosphere that degrades astronomical images
differential rotation
Poor Cluster
tectonics of Venus
Light Pollution
6. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
CNO Cycle
nucleus
Neutron Star
Cassini division
7. Electromagnetic Radiation
condensation temperature
A family of radiant energy- includes light
Positive - Converge - Greater than 1
mass
8. The entity from which the whole universe is postulated to have come from.
cosmic singularity
Turn off Point
aphelion
zone
9. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
MOONS: most geologically active
isotropic
Absorption Spectrum
rotation curve=winding dilemma?
10. All possible types of energy that can be emitted and absorbed by atoms.
jovian
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.
Plague
Electromagnetic Radiation
11. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
isotropic
cosmological principle
Rich vs poor clusters
Apollo asteroids
12. The rock that makes up the lunar maria
planetary nebula
mare basalt
Hubble constant
Dark Nebula
13. The place in the sky that the Earth's axis points toward (can be either north or south)
Primary Mirror
Colestial Pole
Photon
slowest rotation
14. Theory virtually demands that the geometry of the universe be ______. Results of measuring lumps in the cosmic background radiation indicate that the universe geometry is ________.
greatest elongation
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.
OB Associations
Flat - Flat
15. Any change in the speed or direction of an object's motion
White Dwarf
The Big Bang Theory resolves Olber's Paradox
Ole Roemer
acceleration
16. Earth
protostar
Most dense
aurora
Meridian
17. A collection of galaxies like the one the Milky Way belongs to
SETI
Poor Cluster
Self-Propogating Star Formation
direct motion
18. An entity that is likely in the nucleus of most - if not all - galaxies.
acceleration
supermassive black hole
comet
CNO Cycle
19. A planet orbiting about a distant star
zone
Extrasolar Planet
Electromagnetic Radiation: Ultraviolet Light
Gravitational Lens
20. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Parallax
Neutron Star
mare basalt
terrestrial planet
21. The part of the Milky way that has on-going star formation
CNO Cycle
Disk
Particle Horizon
partile horizon
22. 100 nm 10 nm
Supercluster
Wein's Law
Electromagnetic Radiation: Ultraviolet Light
Pixel
23. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
asteroid
Poor Cluster
accretion
Ganymede (Jupiter)
24. Material that shoots rapidly out into space. Flares cause Auroras
Halo
Planetary Nebula
most eccentric orbit
Flare
25. A method of finding a star's distance from its absolute magnitude and spectral type or color.
great red spot
Spectroscopic Parallax
Ganymede (Jupiter)
Degeneracy
26. A force exerted by reflecting sunlight
belt
Photon
radiation pressure
Population 1 vs Population 2 stars
27. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
3 reasons we orbit satellites to observe universe
quarks
Primary Mirror
CCD
28. When one side of a body always faces the planet it revolves around
most moons
chemical differentiation
Celestial Sphere
synchronous rotation
29. The normal eastward movement of a planet against the background of hte distant stars.
Proton-proton chain
White Dwarf
radiation dominated universe
direct motion
30. 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
synchrotron radiation
Hubble law
Ole Roemer
Asymptotic giant Branch Star
31. The location in the Milky Way where stars orbit like a solid wheel
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Light Curve
widmanstatten pattern
Bulge
32. A volume of space where few - if any - galaxies are located
most eccentric orbit
chemical differentiation
Void
Positive - Converge - Greater than 1
33. Long - meandering cliff formed when a planet surface cools and shrinks
scarp
coma
Kirchhoff's Law
HII Region
34. A huge sphere of tenuous gas surrounding the nucleus of a comet
Positive - Converge - Greater than 1
Main Sequence Stars
coma
belt
35. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Callisto (Jupiter)
Cepheid Variable
Flare
Supernova (You can be my supernova girl)
36. 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.
Autumnal Equinox
Apparent Magnitude
open star clusters
scarp
37. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Hubble constant
MOONS: roundest shape
If it is in a denser medium - such as glass - it will move slower
Supercluster
38. Why do Galaxies move very rapidly in the interiors of the dense clusters?
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
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
contrast northern lowlands and the southern highlands of mars...
reflection star clusters
39. A plot of star absolute magnitude verses spectral type.
Electromagnetic Radiation: X-Ray
Photon
E=mc2
H-are Diagram
40. 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.
Population 1 vs Population 2 stars
mapping the structure of Milky Way disk
Planetary Nebula
Cosmic Microwave Background (CMB)
41. Jupiter - Saturn - Uranus - Neptune
Jovian Planets
Gamma-ray Burst
Negative - Diverge - Less than 1
coma
42. VENUS
protostar
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
High Velocity Stars
Spectral Lines
43. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
most moons
density parameter
Synodic Day
H2 Regions
44. The science of measuring light energy by wavelength.
Void
A family of radiant energy- includes light
H-are Diagram
Spectroscopy
45. The north-south line passing directly overhead through the zenith.
Meridian
Parsec
resonance
Synodic Day
46. A star that is burning hydrogen to helium in a shell surrounding it's core
Red Giant Branch Star
Limb darkening
Yes - frozen at the poles- remains protected from the suns rays
Photon
47. 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
force
Light Curve
retrograde motion
48. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
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.
HII Region
fastest rotation
Absolute Magnitude
49. A streak of light in the atmosphere
Supercluster
meteor
Open Cluster
inferior planets
50. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Active Optics
density parameter
Cassini division
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.
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