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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. 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
Most dense
Spectroscopic parallax
Black Hole
Cassegrain Focus
2. What do we think the actual fate of the universe will be and why do we think this?
Steady State Theory (Leads to Olber's Paradox)
Sb spiral galaxy
isotropic
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.
3. The entity responsible for spiral arms in grand-design spiral galaxies
Instability strip
Turn off Point
Density Wave
Proton-proton chain
4. When a planet lines up with the sun inthe sky
conjunction
widmanstatten pattern
Seyfert galaxy
Sc spiral galaxy
5. Jupiter
Largest diameter
Stephen-Boltzman Law
Main Sequence Stars
synchrotron radiation
6. A particle of light.
Photon
Annular Eclipse
chemical differentiation
Active Optics
7. Flat disk with gas - dust - H2 regions - molecular clouds - dust young stars and remnants of old planetary nebula and supernova remnants. stars spin together with similar velocities called differential rotation
partile horizon
Electromagnetic Radiation: Gamma Ray
tectonics of Venus
disk
8. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
If it is in a denser medium - such as glass - it will move slower
great dark spots
meteor
tectonics of Mars
9. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Summer Solstice
chondrite
quasar
Turn off Point
10. Small moons that maintain the shape of rings around Saturn and Uranus
Shepherd satellite
Spectroscopic parallax
3 reasons we orbit satellites to observe universe
matter dominated universe
11. The point in its orbit where a planet is farthest from the sun
Ionization
radiation pressure
Apparent Magnitude
aphelion
12. The sinking of denser elements to the center of a young molten planet
chemical differentiation
Negative - Diverge - Less than 1
Bulge
Atomic Number
13. IO
Largest diameter
Perihelion
era of recombination
MOONS: most geologically active
14. A star that erratically and explosively brightens and dims
Nova
radio lobe
Enke gap
mapping the structure of Milky Way disk
15. The mass of an object divided by its volume
Nova
density
highlands
Neutron Star
16. The time when the universe cooled sufficiently for atoms to exist. radiation dominated= first 300000 years - THEN era of recombination turns into matter dominated for next.
era of recombination
Grand design spirals
Interstellar Extinction
cosmological red shift
17. When massive objects bend space and time enough to create multiple images of an object located behind them
Gravitational Lens
Yes - frozen at the poles- remains protected from the suns rays
Zenith
Gamma-ray Burst
18. A word used in astronomy to describe all elements besides hydrogen and helium
Metals
radiation pressure
Cepheid Variable
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
19. 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.
Rich Cluster
Spectroscopic Parallax
Oort Cloud
Nova
20. 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.
Oort Cloud
H2 Regions
Interstellar Extinction
Electromagnetic Radiation: Ultraviolet Light
21. Possible Fates of the Universe
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
Neutron Star
Light: travels like a wave - detected like a particle
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
22. 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
superclusters
Nucleus
greatest elongation
Spectroscopic parallax
23. The organization of clusters of galaxies into sheets and strings
Supercluster
Hydrostatic Equilibrium
thinnest atmosphere
fewest moons
24. The elementary building blocks from which protons and neutrons are formed.
quarks
aphelion
Nebula
Kuiper belt
25. The act of removing an electron from an atom.
quarks
Electromagnetic Radiation: X-Ray
most moons
Ionization
26. A small and dim but hot star.
White Dwarf
Degeneracy
Celestial Sphere
difference between maria and highlands of the moon.
27. Mercury
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
cosmic singularity
300000 KM/sec
thinnest atmosphere
28. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
interstellar dust
density
Pulsar
Molecular Clouds
29. 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.
nucleus
Yes - frozen at the poles- remains protected from the suns rays
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Cassini division
30. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
planetary nebula
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.
rotation curve=winding dilemma?
Jupiters red spot
31. Originially thought to be stars emitting radio radiation but are now concluded to be nuclei of distant galaxies (same as radio galaxies aka emit streams of material)
quasar
Bok Globule
radiation pressure
Maria
32. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Radiative Diffusion
Emission Spectrum
tectonics of Earth
MOONS: largest size
33. An element of a highly efficient - two-dimensional electronic light detector
Pixel
mapping the structure of Milky Way disk
Primary Mirror
coma
34. 10 nm 10^2 nm
least dense
accretion
Focal Plane
Electromagnetic Radiation: X-Ray
35. A streak of light in the atmosphere
MOONS: largest size
Light Curve
meteor
Open - flat - and closed.
36. A word meaning 'the same everywhere throughout.'
homogeneous
mare basalt
HII Region
roche limit
37. The distance light travels in one year (=9.46x10^12km).
Light-Year
deferent
Apollo asteroids
Vernal Equinox
38. An entity that is likely in the nucleus of most - if not all - galaxies.
Refractor
supermassive black hole
Geocentric
Flocculent spirals
39. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
quasar
3 reasons we orbit satellites to observe universe
Liquid metallic hydrogen
Terrestrial Planets
40. The science of measuring light energy by wavelength.
Spectroscopy
Instability strip
Light-Year
Make up of the jovian planets
41. The high- temperatature outer layer of the sun
Corona
Liquid metallic hydrogen
Plague
Summer Solstice
42. The apparent backward motion of a planet against the background of stars.
If it is in a denser medium - such as glass - it will move slower
retrograde motion
radiant
Gamma-ray Burst
43. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
Grand design spirals
fusion crust
Kirkwood gaps
scarp
44. A two-filter measure of the color - and hence temperature - of a star.
Color Index
tectonics of Venus
Energy Level
SETI
45. When material is heated and moves taking the heat energy with it
CCD
disk
Light: travels like a wave - detected like a particle
Convection
46. Venus
rotation curve=winding dilemma?
Cepheid variables
Quasar
hottest surface
47. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
Dark matter candidates
radio galaxy
terrestrial planet
Seyfert galaxy
48. A very dense - highly populated cluster of galaxies
difference between maria and highlands of the moon.
Degeneracy
Cosmic Microwave Background
Rich Cluster
49. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
CCD
semimajor axis
Dark matter candidates
interstellar dust
50. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Summer Solstice
Make up of the terrestrial planets
weight
Nebula