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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 huge sphere of tenuous gas surrounding the nucleus of a comet
High Velocity Stars
partile horizon
Stephen-Boltzman Law
coma
2. The mirror that determines the focus configuration of a reflector
Supernova (You can be my supernova girl)
Secondary Mirror
Sb spiral galaxy
accretion
3. Earth
Radio Galaxy
differential rotation
Ole Roemer
Most dense
4. An evolved star - past the helium flash that is burning helium to carbon in it's cores
radiation dominated universe
roche limit
Horizontal Branch Star
radiant
5. A location on an H-are Diagram where evolving stars pulsate
great dark spots
Granules
Kuiper belt
Instability strip
6. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
protostar
blazar
interstellar dust
Neutron Star
7. Wave- only waves cause an interference pattern when passing through a double slit - particle- only particles deposit energy at specific locations (the way an image builds up on digital camera)
Light: travels like a wave - detected like a particle
density waves
Granules
Self-Propogating Star Formation
8. A small and dim but hot star.
acceleration
White Dwarf
Kuiper belt
quasar
9. The 'edge' of the universe. Light beyond this has not reached us yet.
partile horizon
Titus-Bode Law
CNO Cycle
Differential Rotation
10. A word used in astronomy to describe all elements besides hydrogen and helium
radio lobe
Metals
Dark Matter
Eclipses of the Moons of Jupiter
11. As open clusters age - they push gas away but dust remains this can reflect light giving the cluster a blue-ish color. also called reflection nebula
reflection star clusters
planetesimal
E=mc2
radiant
12. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
SETI
Rich vs poor clusters
Degeneracy
CCD
13. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
shape and color of SPIRAL galaxies
Callisto (Jupiter)
300000 KM/sec
Jovian Planets
14. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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15. 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
interstellar dust
reflection star clusters
Kuiper belt
force
16. The location of a supermassive black hole
Ground State
Nucleus
Open Cluster
quarks
17. The process of acquiring material
accretion
Planetary Nebula
Largest diameter
Flat - Remain Parallel - Exactly 1
18. 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
Asymptotic giant Branch Star
Electromagnetic Radiation: Radio
Dark Nebula
Flat - Remain Parallel - Exactly 1
19. Young clusters in disk are irregularly shaped since they have no time to relax into the rounder relaxed shape of globular clusters-will constantly be torn apart and assimilated.
Hubble constant
Negative - Diverge - Less than 1
open star clusters
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
20. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
Planck time
Radio Galaxy
Hubble constant
MOONS: largest size
21. The 'edge' of the universe. Light beyond this has not reached us yet.
partile horizon
Sa spiral galaxy
Jupiters red spot
Electromagnetic Radiation: Visible Light
22. The gap etween saturn's A and B rings
Cassini division
Refractor
Zenith
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.
23. Venus
Total Eclipse
Flare
Thickest atmosphere
Magnification
24. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
regolith
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
Roundest orbit
rotation curve=winding dilemma?
25. A quantity measuring the stability of the Earth's atmosphere
Black Hole
Seeing
Milky way Galaxy
Open - flat - and closed.
26. 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
disk
Jupiters red spot
Horizontal Branch Star
HII Region
27. Jupiter
Neutron Star
Poor Cluster
Ammonia - methane - and water
most moons
28. A prominence seen against the disk of the sun
aphelion
Gamma ray bursts
Filament
Atomic Number
29. The layer of the sun just above the photosphere
Chromosphere
Celestial Sphere
Focal Plane
Cepheid Variable
30. The oldest terrain on the moon
Spectral Lines
Seeing
Light Gathering Power
highlands
31. When a planet lines up with the sun inthe sky
Open Cluster
3 reasons we orbit satellites to observe universe
Milky way Galaxy
conjunction
32. The family of radiant energy that includes light as a subset
Dark Matter
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
most moons
Electromagnetic Radiation
33. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Pixel
Cosmic Microwave Background (CMB)
Kirchhoff's Law
rotation curve=winding dilemma?
34. The elementary building blocks from which protons and neutrons are formed.
quarks
Light Gathering Power
Planetary Nebula
Planetary Nebula
35. Jupiter - Saturn - Uranus - Neptune
Continuous Spectrum
comet
Spectral Lines
Jovian Planets
36. Centered on the Earth
300000 KM/sec
Geocentric
Spectroscopic parallax
Objective Lens
37. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
Grand design spirals
Flat - Remain Parallel - Exactly 1
Milky way Galaxy
Halo
38. How is the Hubble Law consistent with an expanding universe?
H2 Regions
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.
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
300000 KM/sec
39. A spread of light with an uninterrupted wavelength distribution of energy.
Continuous Spectrum
greehouse effects
Chromosphere
tectonics of Mars
40. A particle of light
Photon
Geocentric
era of recombination
Neutron Star
41. A term referring to Jupiter-like planets
Apollo asteroids
jovian
Sunspots
CCD
42. Long - meandering cliff formed when a planet surface cools and shrinks
meteorite
scarp
Celestial Sphere
Cepheid variables
43. Ganymede and Titan
MOONS: larger than mercury
Shepherd satellite
density waves
Roundest orbit
44. The shadow behind the Earth or Moon where the Sun is partially obscured.
Trojan asteroids
Penumbra
Void
Cassini division
45. A small chunk of rock in space
Big Bang
differential rotation
meteoriod
MOONS: most geologically active
46. The rotation of a star or planet at different speeds at its equator and poles
differential rotation
Parallax
A family of radiant energy- includes light
Color Index
47. 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)
Largest diameter
quasar
Autumnal Equinox
Absolute Magnitude
48. A change in the appearance of the sun at the edge of the solar disk
Yes - frozen at the poles- remains protected from the suns rays
Limb darkening
Zenith
dark matter
49. 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.
hottest surface
Sa spiral galaxy
tectonics of Mars
Maria
50. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Pulsar
widmanstatten pattern
Light-Year
Thermal Equilibrium
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