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Test your basic knowledge |
Cosmology
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Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
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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. 1. We see rapid movements or high energy radiation coming at some level from the nuclei of nearly every galaxy we have looked at. 2. We suspect that the creation of these supermassive black holes is part of the galaxy formation process.
weight
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
neutrino
Galilean satellite
2. A rock or iron specimen that has fallen from space
meteor
belt
meteorite
supermassive black hole
3. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
reflection star clusters
Filament
Electromagnetic Radiation: Visible Light
radio galaxy
4. Collections of young - hot stars
OB Associations
Stephen-Boltzman Law
Shepherd satellite
rotation curve=winding dilemma?
5. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
The Local Group
Flare
comet
Spectral Lines
6. 100 nm 10 nm
Electromagnetic Radiation: Ultraviolet Light
nova
Void
radiation dominated universe
7. Light scattered through the atmosphere that degrades astronomical images
synchrotron radiation
Callisto (Jupiter)
Light Pollution
Europa (Jupiters moon)
8. The location in the Milky Way where stars orbit like a solid wheel
Bulge
Hipparchus
tectonics of Venus
Nebula
9. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
Spectroscopic Parallax
Sunspot cycle
Annular Eclipse
shape and color of ELLIPTICAL galaxies
10. Sc galaxies
Flocculent spirals
asteroid
Electromagnetic Radiation
open star clusters
11. A word meaning 'the same everywhere throughout.'
homogeneous
Photon
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.
Thermonuclear Fusion
12. 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.
Eyepiece Lens
Positive - Converge - Greater than 1
CMB
difference between maria and highlands of the moon.
13. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
CCD
Penumbra
Dark Nebula
Umbra
14. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Corona
Focal Plane
Dark matter candidates
dark energy
15. The process of acquiring material
Perihelion
accretion
Drake equation
Geocentric
16. A telescope that uses mirrors to focus light
Reflector
Hydrostatic Equilibrium
If it is in a denser medium - such as glass - it will move slower
cosmological principle
17. 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.
chondrite
Continuous Spectrum
cosmology
Oort Cloud
18. 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.
Europa (Jupiters moon)
planetesimal
Oort Cloud
synchronous rotation
19. Centered on the Earth
Geocentric
White Dwarf
Open Cluster
chondrite
20. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
solar nebula
Electromagnetic Radiation
Planck time
Reflector
21. The law that describes the blackbody curve - and let to quantum mechanics.
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183
22. When massive objects bend space and time enough to create multiple images of an object located behind them
Parsec
High and low pressure which stretch into bands due to the rapid differential rotation. deeper - darker colors are in the belts and zones are lighter
Dark Matter
Gravitational Lens
23. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Atomic Number
neutrino
Big Crunch
quarks
24. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
Density Wave
comet
Ole Roemer
Make up of the terrestrial planets
25. Earth
Most dense
Kirkwood gaps
radio lobe
Planetary Nebula
26. The elementary building blocks from which protons and neutrons are formed.
MOONS: thickest atmosphere
quarks
Resolving Power
semimajor axis
27. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
mass
radiant
shape and color of SPIRAL galaxies
Plank's Law
28. The crust of a meteorite caused by its entry into Earth's atmosphere
Radiative Diffusion
fusion crust
acceleration
Sc spiral galaxy
29. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
Convection
Io (jupiters moon)
tectonics of Venus
homogeneous
30. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
deferent
Dark Matter
mass
Black Hole
31. IO
Superior planets
fusion crust
meteor shower
MOONS: most geologically active
32. A method of finding a star's distance from its absolute magnitude and spectral type or color.
radiant
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.
rotation curve=winding dilemma?
Spectroscopic Parallax
33. The first rock-sized bodies that formed in the solar nebula from dust grains
direct motion
chondrite
cosmic fireball
Asymptotic giant Branch Star
34. The study of the universe as a whole.
Hubble law
meteor shower
cosmology
fusion crust
35. 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.
SETI
density parameter
open star clusters
partile horizon
36. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Stephen-Boltzman Law
Continuous Spectrum
Negative - Diverge - Less than 1
most moons
37. Moon in less than the angular diameter of the Sun.
quarks
Ganymede (Jupiter)
Electromagnetic Radiation: Infrared
Annular Eclipse
38. The law that syas light energy from a blackbody increases as (temperature^4)
Primary Mirror
Stephen-Boltzman Law
planetesimal
Self-Propogating Star Formation
39. Elliptical orbits that come inside orbit of the Earth.
Inverse Square Law
homogeneous
Seeing
Apollo asteroids
40. A massive variable star used to find distances to the galaxies or clusters that contain them.
Cepheid Variable
radiation dominated universe
Ecliptic
terrestrial planet
41. What do we think the actual fate of the universe will be and why do we think this?
Neutron Star
Photosphere
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.
Colestial Pole
42. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Photon
Neutron Star
The Local Group
smallest diameter
43. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Kirkwood gaps
Chromosphere
Poor Cluster
Nucleus
44. The normal eastward movement of a planet against the background of hte distant stars.
Turn off Point
evidence of water on mars
zone
direct motion
45. How is the Hubble Law consistent with an expanding universe?
Light-Year
Active Optics
most moons
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.
46. Then the Sun moves from north to south across the celestial equator (about September 23)
CNO Cycle
Plank's Law
Autumnal Equinox
High and low pressure which stretch into bands due to the rapid differential rotation. deeper - darker colors are in the belts and zones are lighter
47. Either Io -Europa - Ganymede - or Callisto
Galilean satellite
Blackbody Curve
jovian
Eyepiece Lens
48. How is the Hubble Law consistent with an expanding universe?
Ole Roemer
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.
Electromagnetic Radiation: Microwave
Hyashi track
49. A location on an H-are Diagram where evolving stars pulsate
Convection
Cosmic Microwave Background (CMB)
Instability strip
epicycle
50. When a planet lines up with the sun inthe sky
conjunction
Milky way Galaxy
Electromagnetic Radiation: Infrared
Halo
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