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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. A star that is burning hydrogen to helium in a shell surrounding it's core
Blackbody
epicycle
Red Giant Branch Star
OB Associations
2. VENUS
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
Summer Solstice
Oort cloud
condensation temperature
3. A term referring to Jupiter-like planets
jovian
Neutron Star
Electromagnetic Radiation: Ultraviolet Light
Annular Eclipse
4. In a FLAT UNIVERSE(our universe) - the curvature of space-time is ________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
OB Associations
Positive - Converge - Greater than 1
Flat - Remain Parallel - Exactly 1
neutrino
5. An entity that is likely in the nucleus of most - if not all - galaxies.
Ground State
opposition
Reflector
supermassive black hole
6. A term referring to the orbital character of stars near the Sun
Differential Rotation
roche limit
Disk
Summer Solstice
7. Distance from sun to nucleus- 8 kiloparsecs (26000 LY) - diameter of Milky way- 150000 LY - length for sun to orbit once around milky way- 250 million years
CMB
Milky way Galaxy
contrast northern lowlands and the southern highlands of mars...
Rich vs poor clusters
8. The layer of the sun just above the photosphere
Chromosphere
Rich Cluster
Drake equation
smallest diameter
9. The north-south line passing directly overhead through the zenith.
Kirkwood gaps
Meridian
Thickest atmosphere
Geocentric
10. Matter so dense that even light cannot escape its gravity
Inverse Square Law
Black Hole
Kirkwood gaps
isotropic
11. A change in the wavelength of light caused by a motion between the observer and light (or wave) source (blue shift if getting closer - red shift if moving away)
300000 KM/sec
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Doppler Shift
Lagrangian Razor
12. The process of acquiring material
Maria
accretion
Quasar
Differential Rotation
13. The location in an H-are diagram of a star cluster - where stars have just left the main sequence. Used to estimate the cluster age.
nucleus
slowest rotation
Turn off Point
deferent
14. A two-filter measure of the color - and hence temperature - of a star.
quarks
Electromagnetic Radiation: Gamma Ray
Color Index
How is winding dilemma solved?
15. The telescope configuration that has the focus placed at the back of the primary mirror
Cassegrain Focus
quasar
opposition
Blackbody Curve
16. Venus (retrograde)
Photon
slowest rotation
comet
Astronomical Unit
17. Saturn
least dense
blazar
weight
Self-Propogating Star Formation
18. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Parallax
great dark spots
Brown dwarf
Oort cloud
19. The organization of clusters of galaxies into sheets and strings
force
Liquid metallic hydrogen
Olber's paradox
Supercluster
20. Is there water on the moon?
fusion crust
Yes - frozen at the poles- remains protected from the suns rays
Focal Length
inferior planets
21. The process that powers the sun and hydrogen bombs
Thermonuclear Fusion
Photosphere
Enke gap
Colestial Pole
22. Dark areas on the sun that are cooler than the surrounding photosphere
Sunspots
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Filament
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
23. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
Ground State
H2 Regions
AGN
blazar
24. A collection of galaxies like the one the Milky Way belongs to
Poor Cluster
Planetary Nebula
regolith
Electromagnetic Radiation: Microwave
25. The rock that makes up the lunar maria
Extrasolar Planet
mare basalt
Sb spiral galaxy
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.
26. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Summer Solstice
Sc spiral galaxy
Wein's Law
Flocculent spirals
27. The first rock-sized bodies that formed in the solar nebula from dust grains
Electromagnetic Radiation: Radio
chondrite
Largest diameter
partile horizon
28. Long - meandering cliff formed when a planet surface cools and shrinks
Interstellar Extinction
Asymptotic giant Branch Star
deferent
scarp
29. 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
Primary Mirror
Spectral Lines
Superior planets
30. Poitns of gravitational stability in the orbit of a planet
inferior planets
Lagrangian Razor
Nova
Largest diameter
31. Hydrogen and helium (mainly)
Make up of the jovian planets
gravity
Winter Solstice
Planck time
32. Collections of young - hot stars
MOONS: most geologically active
MOONS: thickest atmosphere
Thickest atmosphere
OB Associations
33. Small moons that maintain the shape of rings around Saturn and Uranus
partile horizon
Rich vs poor clusters
Shepherd satellite
Globular Cluster
34. Finding a star's absolute magnitude from it's placement on an HR diagram. After finding the absolute magnitude - we measure the apparent magnitude - for a distance modulus and use this to find the distance. This method is good for finding distances t
Spectroscopic parallax
Brown dwarf
fastest rotation
Hyashi track
35. The normal eastward movement of a planet against the background of hte distant stars.
direct motion
thinnest atmosphere
Reflector
planetesimal
36. The location in the Milky Way where stars orbit like a solid wheel
Limb darkening
deferent
Filament
Bulge
37. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
condensation temperature
Secondary Mirror
density waves
planetesimal
38. First accurately measured the speed of light in a vacuum
SETI
300000 KM/sec
Ole Roemer
Ganymede (Jupiter)
39. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Dark Nebula
Olber's paradox
Convection
cosmic fireball
40. The shadow behind the Earth or Moon where the Sun is partially obscured.
direct motion
Penumbra
Spectral Lines
self-propagating star formation
41. The philosophical stand that says a simpler explanation is more likely to be correct than a complicated one.
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42. VENUS
Thermal Equilibrium
planetary nebula
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
Emission Spectrum
43. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Olber's paradox
Horizontal Branch Star
Big Crunch
MOONS: largest size
44. When the Sun moves from south to north across the celestial equator (about March 21)
Instability strip
Plague
Vernal Equinox
3 reasons we orbit satellites to observe universe
45. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
molecular clouds
Granules
cosmological red shift
radio lobe
46. When the Sun is farthest south of the celestial equator (About December 22)
Winter Solstice
terrestrial planet
Thickest atmosphere
Density Wave
47. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
Sunspot cycle
Autumnal Equinox
bulge
most moons
48. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Light Pollution
evidence of water on mars
critical density
Spectroscopic Parallax
49. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Wein's Law
semimajor axis
synchrotron radiation
cosmic singularity
50. Mercury
Make up of the jovian planets
condensation temperature
Parsec
most eccentric orbit