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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. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
OB Associations
Supernova (You can be my supernova girl)
planetesimal
Kuiper belt
2. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
Black Hole
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.
dark energy
Spectroscopic Parallax
3. The light produced when particles from the sun collide with atmospheric molecules
rotation curve = dark matter?
Kuiper belt
High Velocity Stars
aurora
4. A huge sphere of tenuous gas surrounding the nucleus of a comet
Heliocentric
Radio Galaxy
bulge
coma
5. A star that has become a red giant for the second and final time. It is burning helium to carbon in a shell surrounding the core
Spectroscopic Parallax
Asymptotic giant Branch Star
Focal Plane
cosmological principle
6. The entity responsible for spiral arms in grand-design spiral galaxies
accretion disk
Particle Horizon
Rich Cluster
Density Wave
7. Star speed at outer edge of galaxy should begin to diminish - but they dont so we guess that this means there is increasing force (aka dark matter)
rotation curve = dark matter?
Eyepiece Lens
condensation temperature
radio galaxy
8. The rotation of a star or planet at different speeds at its equator and poles
differential rotation
MOONS: roundest shape
Void
Ecliptic
9. The dark - relativley smooth areas on the moon; Latin for sea
cosmic fireball
Eyepiece Lens
belt
Maria
10. A plot of star absolute magnitude verses spectral type.
Proton-proton chain
H-are Diagram
Objective Lens
cosmic fireball
11. The wavelengths where a specific element can absorb or emit light.
How is winding dilemma solved?
White Dwarf
open star clusters
Spectral Lines
12. Jupiter
Largest diameter
Continuous Spectrum
Liquid metallic hydrogen
AGN
13. 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
CCD
Photon
High Velocity Stars
Oort cloud
14. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Perihelion
The Local Group
Plague
Kirkwood gaps
15. The elementary building blocks from which protons and neutrons are formed.
quarks
Red Giant Branch Star
Make up of the jovian planets
quasar
16. The north-south line passing directly overhead through the zenith.
Steady State Theory (Leads to Olber's Paradox)
Precession
mapping the structure of Milky Way disk
Meridian
17. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
planetary nebula
belt
Wein's Law
comet
18. 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)
meteor shower
inferior planets
Electromagnetic Radiation: X-Ray
quasar
19. First accurately measured the speed of light in a vacuum
chondrite
Ole Roemer
evidence of water on mars
Sa spiral galaxy
20. The source of the force that is accelerating the expansion rate of the universe.
dark energy
Bok Globule
rotation curve=winding dilemma?
The Big Bang Theory resolves Olber's Paradox
21. A galaxy emitting large amounts of energy at long wavelengths.
Ionization
radio galaxy
Sunspot cycle
Asymptotic giant Branch Star
22. Long - meandering cliff formed when a planet surface cools and shrinks
Density Wave
Electron
scarp
Rich Cluster
23. The process responsible for creating the arms of flocculent spiral galaxies
Molecular Clouds
Corona
Cassegrain Focus
Self-Propogating Star Formation
24. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Neutron Star
Titus-Bode Law
nova
Dark Nebula
25. A spectrum of light with energy at only a few wavelengths.
quasar
Emission Spectrum
cosmological red shift
Supercluster
26. How is the Hubble Law consistent with an expanding universe?
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.
Nova
Sunspot cycle
Eclipses of the Moons of Jupiter
27. The crust of a meteorite caused by its entry into Earth's atmosphere
Sc spiral galaxy
fusion crust
reflection star clusters
Rich Cluster
28. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
rotation curve=winding dilemma?
bulge
H-are Diagram
Electromagnetic Radiation: Visible Light
29. A telescope that uses mirrors to focus light
Gamma ray bursts
Light-Year
Reflector
mapping the structure of Milky Way disk
30. 1μm 100 nm
Nebula
Electromagnetic Radiation: Visible Light
Self-Propogating Star Formation
belt
31. The layer of the sun just above the photosphere
disk
Kuiper belt
Energy Level
Chromosphere
32. A phenomenon seen when the Earth passes through the orbit of a burned out comet
dark energy
meteorite
meteor shower
Electromagnetic Radiation
33. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Coronal Loop
Bulge
quasar
smallest diameter
34. A bridge of material held in position above the solar surface. They can remain for hours even days
accretion disk
aurora
Prominence
Granules
35. A rock or iron specimen that has fallen from space
dark matter
Particle Horizon
greehouse effects
meteorite
36. The 'edge' of the universe. Light beyond this has not reached us yet.
partile horizon
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
Lagrangian Razor
Plague
37. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
general star population
Absolute Magnitude
Sa spiral galaxy
Planck time
38. Jupiter
most moons
zone
standard candle
era of recombination
39. The dimming of starlight by intervening dust
Interstellar Extinction
bulge
coma
Seeing
40. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
radio galaxy
retrograde motion
Primary Mirror
opposition
41. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
Dark matter candidates
Particle Horizon
opposition
asteroid
42. The apparent path of the Sun through the stars on the celestial sphere.
Ecliptic
Limb darkening
open star clusters
Hubble law
43. The shadow area behind the Earth or Moon where the Sun is completely obscured.
retrograde motion
Kuiper belt
Umbra
3 reasons we orbit satellites to observe universe
44. The process similar to conduction by which energy moves from the solar core to the convective layer
Radiative Diffusion
difference between maria and highlands of the moon.
Prominence
Sidereal Day
45. 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
Hubble law
Zenith
Self-Propogating Star Formation
MOONS: largest size
46. Norhern lowlands- darker in color and have far fewer craters as if an ancient sea or ice field covered them. southern highlands- much higher in density of craters.
Active Optics
contrast northern lowlands and the southern highlands of mars...
critical density
force
47. The telescope configuration that has the focus placed at the back of the primary mirror
300000 KM/sec
Geocentric
Cassegrain Focus
Plank's Law
48. The rate of expansion of the universe.
Hubble constant
Annular Eclipse
Pixel
Kirchhoff's Law
49. 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)
Sunspots
Photon
planetary nebula
Focal Plane
50. We can infer the absolute magnitude of pulsating variable stars by measuring their pulsation periods. The longer the pulsations - the greater their luminosities. We then again measure their apparent magnitudes - compare it with their absolute magnitu
Cepheid variables
evidence of water on mars
neutrino
Cosmological Principle
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