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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. Hydrogen and helium (mainly)
opposition
Pulsar
Dark Nebula
Make up of the jovian planets
2. A word meaning 'the same everywhere throughout.'
homogeneous
neutrino
Black Hole
Asymptotic giant Branch Star
3. Population 1- similar to the sun and 2% of elements are metal - Population 2- formed before gas was metal- only a fraction of mass is metal.
Planetary Nebula
Granules
Population 1 vs Population 2 stars
Rich Cluster
4. A prominence seen against the disk of the sun
Filament
Electromagnetic Radiation: X-Ray
Triple Alpha rocess
Plank's Law
5. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
cosmic fireball
supernova
A family of radiant energy- includes light
shape and color of SPIRAL galaxies
6. The location of a supermassive black hole
Nucleus
terrestrial planet
300000 KM/sec
tectonics of Earth
7. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
Cosmic Microwave Background (CMB)
Extrasolar Planet
interstellar dust
Rich vs poor clusters
8. Jupiter
most moons
Io (jupiters moon)
Radio Galaxy
aphelion
9. When a planet lines up with the sun inthe sky
conjunction
semimajor axis
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Seeing
10. The distance a moon can be from a planet before shattering from tidal forces
Magnification
deferent
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.
roche limit
11. 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.
Objective Lens
Parallax
Electromagnetic Radiation
radiation pressure
12. The Greek philosopher responsible for making the stellar magnitude scale.
Hipparchus
partile horizon
conjunction
Photon
13. A point in the sky where meteors appear to come from during a shower
accretion
radiant
Celestial Sphere
Bok Globule
14. Mercury
most eccentric orbit
Penumbra
Nebula
Dark matter candidates
15. 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.
Void
Density Wave
open star clusters
radio galaxy
16. The equation that describes how matter equates with energy
E=mc2
Focal Length
Summer Solstice
MOONS: larger than mercury
17. Light scattered through the atmosphere that degrades astronomical images
Occam's razor
Inverse Square Law
Light Pollution
general star population
18. A particle of light.
Instability strip
Photon
fewest moons
Filament
19. A younger cluster of stars - found in the galaxy disk
Electromagnetic Radiation: X-Ray
Make up of the jovian planets
Electromagnetic Radiation: X-Ray
Open Cluster
20. The particle horizon is the farthest we can see. It exists because the universe had a beginning and thus a definite age. Light from distances farther away from the particle horizon have not had time to reach us yet.
Particle Horizon
Color Index
Cassini division
Absolute Magnitude
21. Small compact stars called white dwarfs can have material deposited on their surfaces. In time material heats up and explodes in surface nuclear reaction- star brightens - settles - repeats.
radio galaxy
nova
Kuiper belt
Proton-proton chain
22. Matter that reveals itself only through its gravitational attraction.
Spectroscopic Parallax
dark matter
Energy Level
Roundest orbit
23. When the Moon entirely blocks the Sun.
AGN
Titus-Bode Law
Total Eclipse
Electromagnetic Radiation: Radio
24. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Absolute Magnitude
Cosmic Microwave Background
tectonics of Earth
Thermal Equilibrium
25. The average distance between the Earth and the Sun (=1.5 x10^8km)
Spectroscopy
Astronomical Unit
planetary nebula
E=mc2
26. Dark areas on the sun that are cooler than the surrounding photosphere
Sunspots
SETI
Cepheid variables
rotation curve=winding dilemma?
27. When a planet lines up with the sun inthe sky
conjunction
Dark matter candidates
Dwarf planets
synchrotron radiation
28. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Active Optics
protostar
greatest elongation
Negative - Diverge - Less than 1
29. A galaxy sending out a stream of material from its nucleus
Dark matter candidates
Radio Galaxy
Cepheid Variable
Emission Spectrum
30. Dying small mass stars lose their outer layers in a relatively gentle way - creating a round or bipolar nebula about the star (round like planets)
planetary nebula
Heliocentric
Particle Horizon
Pulsar
31. How is the Hubble Law consistent with an expanding universe?
Interstellar Extinction
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.
supernova
greehouse effects
32. VENUS
SETI
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.
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
Celestial Equator
33. 1 mm 1μm
Electromagnetic Radiation: Infrared
Differential Rotation
Electromagnetic Radiation: Microwave
Electromagnetic Radiation: Radio
34. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
Black Hole
Grand design spirals
meteorite
cosmological red shift
35. A planet that is farther from the sun than the Earth is
Superior planets
cosmology
Electron
acceleration
36. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Make up of the terrestrial planets
dark energy
If it is in a denser medium - such as glass - it will move slower
fastest rotation
37. When the Sun is farthest north of the celestial equator (about June 22)
Summer Solstice
CMB
Ionization
radiant
38. The amount an image is enlarged by a telescope
Magnification
neutrino
Sidereal Day
Electromagnetic Radiation: Gamma Ray
39. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Sa spiral galaxy
3 reasons we orbit satellites to observe universe
Cosmic Microwave Background (CMB)
rotation curve=winding dilemma?
40. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Drake equation
Main Sequence
direct motion
Big Bang
41. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Black Hole
zone
Main Sequence
chondrite
42. The shadow behind the Earth or Moon where the Sun is partially obscured.
Penumbra
opposition
hottest surface
thinnest atmosphere
43. The high- temperatature outer layer of the sun
nucleus
Red Giant Branch Star
Corona
Dark matter candidates
44. The area behind a lens where images are resolved
MOONS: roundest shape
Precession
Focal Plane
cosmological principle
45. The larger bodies that formed early in teh solar nebula that were chemically differentiated
planetesimal
Dark matter candidates
meteoriod
Thermonuclear Fusion
46. The mix of pure photon energy that emerged at the start of the universe.
Rich vs poor clusters
cosmic fireball
smallest diameter
Continuous Spectrum
47. The source of the force that is accelerating the expansion rate of the universe.
differential rotation
dark energy
Maria
Liquid metallic hydrogen
48. 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)
smallest diameter
Synchrotron Rotation
Meridian
H2 Regions
49. A measure of the force of gravity on an object
tectonics of Earth
weight
Density Wave
inferior planets
50. A telescope that uses lenses to focus light
Radio Galaxy
Refractor
least dense
Electromagnetic Radiation: X-Ray
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