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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. The number of protons in an atom.
shape and color of ELLIPTICAL galaxies
Gravitational Lens
Neutron Star
Atomic Number
2. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
Electromagnetic Radiation: Ultraviolet Light
cosmological principle
supernova
Thermal Equilibrium
3. The relation that tells how light dims with distance.
Shepherd satellite
Inverse Square Law
Flare
thinnest atmosphere
4. Centered on the sun.
supernova
Heliocentric
Dwarf planets
Filament
5. Earth
H-are Diagram
Most dense
Eyepiece Lens
mare basalt
6. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Nucleus
acceleration
Sa spiral galaxy
epicycle
7. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Summer Solstice
Active Optics
Enke gap
Flare
8. 10^2 nm 10^7 nm
widmanstatten pattern
Electromagnetic Radiation: Gamma Ray
Supercluster
Seeing
9. The mix of pure photon energy that emerged at the start of the universe.
Chromosphere
cosmic fireball
Spectroscopic Parallax
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
10. Europa
fastest rotation
MOONS: roundest shape
Planetary Nebula
fewest moons
11. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
Triple Alpha rocess
Spectroscopy
shape and color of ELLIPTICAL galaxies
Io (jupiters moon)
12. A volume of space where few - if any - galaxies are located
Void
Oort Cloud
general star population
Big Bang
13. Titan
conjunction
quarks
meteor shower
MOONS: thickest atmosphere
14. A fusion process in which protons build together to form helium
Neutron Star
highlands
Neutron Star
Proton-proton chain
15. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Ground State
cosmological principle
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
3 reasons we orbit satellites to observe universe
16. The process similar to conduction by which energy moves from the solar core to the convective layer
aurora
radio galaxy
H-are Diagram
Radiative Diffusion
17. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Heliocentric
Europa (Jupiters moon)
Light Gathering Power
Extrasolar Planet
18. Then the Sun moves from north to south across the celestial equator (about September 23)
MOONS: most geologically active
A family of radiant energy- includes light
shape and color of SPIRAL galaxies
Autumnal Equinox
19. Small moons that maintain the shape of rings around Saturn and Uranus
Cosmological Principle
Electromagnetic Radiation
cosmic fireball
Shepherd satellite
20. What do we think the actual fate of the universe will be and why do we think this?
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.
synchronous rotation
Molecular Clouds
Open - flat - and closed.
21. The law that syas light energy from a blackbody increases as (temperature^4)
Stephen-Boltzman Law
Autumnal Equinox
Dark Nebula
White Dwarf
22. A logarithmically scaled value for the measured brightness of a star.
radiant
most eccentric orbit
MOONS: largest size
Apparent Magnitude
23. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
density parameter
Ole Roemer
quarks
aphelion
24. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
Gamma ray bursts
planetary nebula
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
25. 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.
Poor Cluster
CMB
weight
Ganymede (Jupiter)
26. A word meaning 'the same everywhere throughout.'
homogeneous
semimajor axis
inferior planets
Supernova (You can be my supernova girl)
27. What Ole Roemer used to measure the speed of light in a vacuum
synchrotron radiation
Eclipses of the Moons of Jupiter
cosmology
Inverse Square Law
28. 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)
Nova
standard candle
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
29. Formed from slow rotating clouds - collapsed quicker - initial star formation rate is high but died out - older - little rotation - look redder
shape and color of ELLIPTICAL galaxies
Flat - Remain Parallel - Exactly 1
Stephen-Boltzman Law
most moons
30. A distance measure determined by the shifting of a star against the background sky every 6 months.
planetary nebula
Reflector
Parsec
fastest rotation
31. That which is responsible for Jupiter's magnetic field
density waves
most moons
Refractor
Liquid metallic hydrogen
32. Large nebula consisting of very cold gas and dust
Radio Galaxy
Light Gathering Power
Molecular Clouds
disk
33. A star that erratically and explosively brightens and dims
Winter Solstice
Nova
widmanstatten pattern
Light Curve
34. Jupiter
most moons
AGN
Spectroscopy
Reflector
35. An empirical scheme for predictin ghe orbital distances of planets
Electromagnetic Radiation: X-Ray
Wein's Law
conjunction
Titus-Bode Law
36. The source of the force that is accelerating the expansion rate of the universe.
Parallax
Absolute Magnitude
dark energy
radio galaxy
37. Ganymede
Lagrangian Razor
MOONS: largest size
slowest rotation
Coldest surface
38. The rotation period of the Earth measured relative to the stars.
Sidereal Day
rotation curve = dark matter?
Superior planets
Electromagnetic Radiation: Visible Light
39. A planet that is farther from the sun than the Earth is
Disk
Superior planets
Thermal Equilibrium
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.
40. The oldest terrain on the moon
Total Eclipse
highlands
shape and color of ELLIPTICAL galaxies
300000 KM/sec
41. The law that predicts the possible types of spectra.
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42. 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
Main Sequence Stars
bulge
Dark Matter
quasar
43. That which is responsible for Jupiter's magnetic field
Astronomical Unit
Perihelion
Liquid metallic hydrogen
Black Hole
44. 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.
tectonics of Venus
Void
fewest moons
CMB
45. 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)
3 reasons we orbit satellites to observe universe
roche limit
H2 Regions
Thermal Equilibrium
46. 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
scarp
Rich vs poor clusters
Hubble law
Supercluster
47. 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
supermassive black hole
Cepheid variables
Cosmic Microwave Background
Parsec
48. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
radiation dominated 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
Enke gap
Parallax
49. The process that powers the sun and hydrogen bombs
Precession
Superior planets
Density Wave
Thermonuclear Fusion
50. 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
Chandrasekhar Limit
Asymptotic giant Branch Star
thinnest atmosphere
Halo