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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 planet that is farther from the sun than the Earth is
widmanstatten pattern
Superior planets
planetary nebula
Dark Nebula
2. How did Earth come to have an oxygen rich atmosphere?
OB Associations
Seyfert galaxy
Pulsar
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.
3. 1μm 100 nm
reflection star clusters
MOONS: thickest atmosphere
asteroid
Electromagnetic Radiation: Visible Light
4. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
supernova
supermassive black hole
Cassini division
hottest surface
5. 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
Limb darkening
Cepheid Variable
MOONS: largest size
6. A planet orbiting about a distant star
Extrasolar Planet
CMB
planetesimal
dark energy
7. The measure of a variable star's apparent magnitude as it brightens and dims with time
shape and color of ELLIPTICAL galaxies
molecular clouds
Light Curve
Spectroscopy
8. When the Sun moves from south to north across the celestial equator (about March 21)
Black Hole
Vernal Equinox
fastest rotation
Light: travels like a wave - detected like a particle
9. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Apollo asteroids
quasar
Sunspots
Gamma ray bursts
10. Population 1- similar to the sun and 2% of elements are metal - Population 2- formed before gas was metal- only a fraction of mass is metal.
Primary Mirror
supernova
Population 1 vs Population 2 stars
mapping the structure of Milky Way disk
11. A rock or iron specimen that has fallen from space
meteorite
Pixel
Lagrangian Razor
Celestial Sphere
12. Distribution of dust (tells us disk is thin) - find distances to O&B stars and H2 regions (arms are sights of star formation and OB stars live and die at location of birth) -Milky way has four arms. Sun is in spur apart from arms.
mapping the structure of Milky Way disk
Oort cloud
evidence of water on mars
Maria
13. The Greek philosopher responsible for making the stellar magnitude scale.
Cepheid Variable
Total Eclipse
Electromagnetic Radiation: X-Ray
Hipparchus
14. The oldest part of the Milky Way
Perihelion
Stephen-Boltzman Law
Halo
hottest surface
15. VENUS
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Ground State
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
Cosmological Principle
16. The rock that makes up the lunar maria
Eclipses of the Moons of Jupiter
Resolving Power
mare basalt
Steady State Theory (Leads to Olber's Paradox)
17. A prominence seen against the disk of the sun
Filament
Vernal Equinox
inferior planets
Horizontal Branch Star
18. The place in the sky that the Earth's axis points toward (can be either north or south)
Colestial Pole
CNO Cycle
radiant
rotation curve = dark matter?
19. Mercury
most eccentric orbit
Cosmological Principle
Blackbody Curve
Population 1 vs Population 2 stars
20. A prominence seen against the disk of the sun
Filament
Dark Matter
epicycle
Terrestrial Planets
21. A spectrum of light with energy at only a few wavelengths.
Emission Spectrum
Plague
tectonics of Mars
Parsec
22. Mercury - Venus - Earth - Mars
Annular Eclipse
Terrestrial Planets
Rich Cluster
reflection star clusters
23. 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.
dark energy
Oort Cloud
Annular Eclipse
Dwarf planets
24. The light produced when particles from the sun collide with atmospheric molecules
Inverse Square Law
Kirkwood gaps
radiant
aurora
25. A representation of the changes in color and brightness of an evolving protostar.
Electromagnetic Radiation: Visible Light
fastest rotation
Callisto (Jupiter)
Hyashi track
26. The equation that describes how matter equates with energy
E=mc2
smallest diameter
thinnest atmosphere
Electromagnetic Radiation: Visible Light
27. Mercury
Parsec
mare basalt
Astronomical Unit
most eccentric orbit
28. In what chemical form are jupiters nitrogen - carbon and oxygen?
Ammonia - methane - and water
Focal Length
supernova
matter dominated universe
29. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
Supercluster
Photon
cosmological principle
Sunspot cycle
30. The mix of pure photon energy that emerged at the start of the universe.
cosmic fireball
Synodic Day
disk
Make up of the terrestrial planets
31. The 'edge' of the universe. Light beyond this has not reached us yet.
partile horizon
MOONS: larger than mercury
greatest elongation
Ground State
32. The dimming of starlight by intervening dust
Interstellar Extinction
Photon
Flat - Flat
Black Hole
33. That which is responsible for Jupiter's magnetic field
Eclipses of the Moons of Jupiter
Apparent Magnitude
meteor shower
Liquid metallic hydrogen
34. The sinking of denser elements to the center of a young molten planet
300000 KM/sec
Gamma ray bursts
Shepherd satellite
chemical differentiation
35. The rotation period of the Earth measured relative to the Sun.
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.
Gamma-ray Burst
Synodic Day
300000 KM/sec
36. The point directly overhead.
anorthosite
Self-Propogating Star Formation
Zenith
Hubble law
37. The era when the ratio of matter to energy greatly favored matter. (verses radiation dominated universe where it was opaque. Matter is now dominated by gravity not photons)
matter dominated universe
cosmic singularity
Largest diameter
Active Optics
38. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
comet
Cepheid variables
Rich vs poor clusters
cosmological principle
39. The wavelengths where a specific element can absorb or emit light.
shape and color of ELLIPTICAL galaxies
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
Astronomical Unit
Spectral Lines
40. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
CCD
Proton-proton chain
Parallax
great dark spots
41. 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
Corona
Kuiper belt
condensation temperature
Nebula
42. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Population 1 vs Population 2 stars
3 reasons we orbit satellites to observe universe
Light Pollution
Thermonuclear Fusion
43. A continuous spectrum of light missing energy at a few wave lengths.
MOONS: most geologically active
gravity
Absorption Spectrum
meteor shower
44. The class of all objects having high energy radiation coming from their nuclei. Active Galactic Nucleus- Blazars - Quasars - Radio and Emit synchrotron radiation
Brown dwarf
mapping the structure of Milky Way disk
AGN
Negative - Diverge - Less than 1
45. The rotation period of the Earth measured relative to the stars.
Drake equation
Disk
Steady State Theory (Leads to Olber's Paradox)
Sidereal Day
46. A word used in astronomy to describe all elements besides hydrogen and helium
zone
protostar
Metals
Electromagnetic Radiation: Infrared
47. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Sidereal Day
Absolute Magnitude
critical density
Chromosphere
48. A planet orbiting about a distant star
Largest diameter
Extrasolar Planet
Poor Cluster
acceleration
49. Material that shoots rapidly out into space. Flares cause Auroras
Electromagnetic Radiation: Microwave
Flare
Doppler Shift
aphelion
50. A faint - remarkably uniform distribution of radiation in space
Cosmic Microwave Background
thinnest atmosphere
Europa (Jupiters moon)
MOONS: larger than mercury