Geology 535 – Early Earth Evolution
Disclaimer: While every reasonable effort is made to ensure that the information provided is accurate, no guarantees for the currency or accuracy of information are made. It takes several proof readings and rewrites to bring the quiz to an exceptional level. If you find an error, please contact me as soon as possible. Please indicate the question ID-Number or description because server may randomize the questions and answers.
Go to: Final Exam
Geology (GLGY 535-UCAL) Midterm Exam
Congratulations - you have completed Geology (GLGY 535-UCAL) Midterm Exam.
You scored %%SCORE%% out of %%TOTAL%%.
Your performance has been rated as %%RATING%%
Question 1 |
A | εNd |
B | εW and εHf |
C | εNd and εHf |
D | εW |
E | εNd and εW |
Question 2 |
A | Major element data are consistent from study to study. |
B | Over 50% of the data on major elements falls considerably outside of the range found by Eade and Fahrig's Canadian Shield Average. |
C | Trace element data are consistent from study to study. |
D | Seismic evidence shows only two parts of the crustal sections; Middle and Lower. The Upper section is distinguished by elemental studies. |
Question 3 |
A | A type of chondrites with high abundance of silica and can be used to measure differentiation time period. |
B | The most primitive chondrites that falls under petrologic Type 1.0 |
C | The most common chondrites that falls under petrologic Type 3.0 to 3.1 |
D | They are part of the differentiated group. |
Question 4 |
A | Within the creaton, platforms are areas where basement is overlaid by sediments and sedimentary rock. |
B | There are only two places on Earth with creatons; Africa and North America. |
C | The geochemical composition of creatons are homogeneous. |
D | Within the creaton, shield are areas where basement is overlaid by sediments and sedimentary rock. |
E | Shield is a made up of several smaller creatonic nuclei. |
Question 5 |
A | Mg |
B | Pb |
C | Cu |
D | S |
E | Al |
Question 6 |
A | 1000 |
B | 5 |
C | 10 |
D | 150 |
Question 7 |
A | Later impacts may have destroyed the raised rim. |
B | Plate tectonics may have destroyed the original structure. |
C | The raised rim is more susceptible to weathering. |
D | Solar radiation and flares may have burnt out the thin and tall rim section. |
Question 8 |
A | Refractory elemental abundance |
B | U-Pb dating |
C | Sm-Nd dating |
D | Fossil evidence |
Question 9 |
A | Heat flux higher than in oceanic domains |
B | Large variations in heat flux within a smaller area |
C | Higher than average heat flux |
D | Lower than average heat flux |
Question 10 |
A | It is easier to determine the isotopic compositions of zircons. |
B | They have hardness of 5 in Mohs scale and therefore resistant to weathering. |
C | They are the most abundant mineral in cratons. |
D | They have a very high closure temperature. |
Question 11 |
A | ...an open system. |
B | ...a closed system. |
C | ...a crustal source. |
D | ...a mantle source. |
E | ...nothing because there is not enough information provided to answer the question. |
Question 12 |
A | 3.69 Ga |
B | 3.69 Ga |
C | 3.55 Ga |
D | 4.56 Ga |
E | 4.23 Ga |
Question 13 |
A | Kaapvaal, South Africa. |
B | Isua Formation, Greenland. |
C | Jack Hill, Australia. |
D | Western Canada Sedimentary Basin, Canada. |
Question 14 |
A | 85% of all Ordinary Chondrites are observed falls. |
B | Most of the Ordinary Chondrites have petrologic types from 3 to 6. |
C | 75% of all Ordinary Chondrites contains CAIs and AOAs. |
D | Ordinary Chondrites are the most common type we have today. |
Question 15 |
A | Venus |
B | Sun |
C | Asteroid belt |
D | Comets |
E | Moon |
Question 16 |
A | Orogenic events |
B | Adiabatic decompression |
C | Interior temperature |
D | Surface P-T conditions |
Question 17 |
A | 8 half-life cycles. |
B | 5 half-life cycles. |
C | 13 half-life cycles. |
D | 14 half-life cycles. |
E | 4 half-life cycles. |
Question 18 |
A | During differentiation of Earth, large portion of silica sank into the core of the Earth. |
B | Differentiation occurs at a extensive rate on larger plants. |
C | All meteorites are not differentiated because they are failed planets. |
D | Differentiation is highly dependent on the pressure conditions. |
Question 19 |
A | Loess |
B | Sandstones |
C | Shale |
D | Limestone |
Question 20 |
A | Any chemical group based on radial distance from the sun |
B | Volatiles, silicates, metal oxides |
C | Silicates, metal oxides, volatiles |
D | Metal oxides, silicates, volatiles |
Question 21 |
A | It is the temperature which 100% of all the elements are condensed out of the nebula gas. |
B | It is the temperature which 100% of a given element is condensed out of the nebula gas. |
C | It is the temperature which 50% of all the elements are condensed out of the nebula gas. |
D | It is the temperature which 50% of a given element is condensed out of the nebula gas. |
Question 22 |
A | ...the sun. |
B | ...in the core of the Earth. |
C | ...in the terrestrial planets. |
D | ...the Earth. |
Question 23 |
A | If most of the samples plots on the concordia. |
B | If some samples plots on the concordia while others on discordia. |
C | If the Pb-loss was episodic/continuous event. |
D | If there is no upper intercept. |
Question 24 |
A | ...an open system. |
B | ...a system that has underwent gradual isotopic gain. |
C | ...a mantle source. |
D | ...a closed system. |
E | ...a crustal source. |
Question 25 |
A | To estimate relationships between cogenetic samples. |
B | To estimate condensation temperatures of materials from Solar Nebula. |
C | To analyze metal-silicate-sulfide differentiation. |
D | To estimate timing of melting and crystallization sequences. |
E | To analyze relatively short processes that occur for 300 million years. |
Question 26 |
A | False because both model and crystallization age are the same. This is how we know the exact age of Earth. |
B | False because the model ages are older than the crystallization ages. |
C | True |
D | Partially true because in most cases model ages are older than the crystallization ages. |
Question 27 |
A | Chemical differentiation due to rapid exothermic reactions. |
B | Migration of molten Fe alloys along grain boundaries of solid silicates. |
C | Differentiation of Fe alloys and silica due to high pressure and temperature conditions. |
D | Heat produced by radioactive isotopes melting the bulk Earth. |
E | Gravitational separation of metallic iron from silicates. |
Question 28 |
A | Loess |
B | Limestone |
C | Shale |
D | Sandstones |
Question 29 |
A | It is the time of primordial soup formation. |
B | It is a standard used to calculate type-sections and GSSPs for Geologic Time boundaries. |
C | It is the time of crystallization. |
D | It is the time of separation of isotope from a given reservoir. |
Question 30 |
A | I. three II. two |
B | I. two II. five |
C | I. two II. four |
D | I. three II. three |
E | I. two II. three |
Question 31 |
A | The system with large number of daughter isotopes ratio most likely have been undergone crustal or magmatic contamination. |
B | The system with large number of daughter isotopes ratio most likely have a steeper isochron. |
C | The system with large number of daughter isotopes ratio most likely have a shallower isochron. |
D | The system with large number of daughter isotopes ratio most likely have been an opened system at some point. |
Question 32 |
A | Could not answer the question because it is depend on the type of setting. |
B | higher than |
C | lower than |
D | same as or very close to |
Question 33 |
A | Sm |
B | Si |
C | Hf |
D | O |
E | Lu |
Question 34 |
A | The closure conditions. |
B | Crystallization age. |
C | Initial isotopic ratio. |
D | The time of formation. |
Question 35 |
A | higher the uncertainties in |
B | larger the diffusion into |
C | larger the diffusion out of |
D | older |
E | younger |
Question 36 |
A | Silica content of the original source of the elements. |
B | Volatility of the elements. |
C | Very high condensation temperature. |
D | Type of reactivity and radioactivity of elements. |
Question 37 |
A | Helium gas |
B | Water vapor |
C | Hydrogen gas |
D | Rocks and dust particles |
Question 38 |
A | Pb-Pb dating of meteorites and pelagic sediment |
B | Hf-W dating of CAI inclusions |
C | Nd model age dating of Isua Supracrustal lithologies |
D | U-Pb dating of meteorites and pelagic sediment |
E | U-Pb dating of ancient zircons |
Question 39 |
A | ...rapidly. |
B | ...extremely slowly. |
C | ...inefficently. |
D | ...in several stages. |
Question 40 |
A | Nobel gases |
B | Silicates |
C | Metal oxides |
D | Ice |
E | Aluminum |
Question 41 |
A | Density of isotopes. |
B | Ratios of parent to daughter isotopes. |
C | Weight and electrical charge of each isotope. |
D | Alpha, beta and positron decay of isotopes. |
Question 42 |
A | electron affinity and reactivity |
B | closure temperature |
C | liquidus temperature |
D | minimum temperature |
E | maximum temperature |
Question 43 |
A | Combination of geochemical and physical analysis of rocks from center and outer rim of the creator. |
B | Overprinting of craters with respect to each other. |
C | Size and shape of the creator. |
D | Geochemical analysis of rocks from the center of the creator. |
Question 44 |
Facies | Profile | Zone |
A1 | Chilled flow top | Spinifex zone |
A2 | Random spinifex | |
A3 | Plate spinifex | |
B1 | - | Cumulate zone |
B2 | - | |
B3 | - |
A | A3 in the plate spinifex region. |
B | Anywhere within the cumulate zone. |
C | B1 |
D | Anywhere within the spinifex zone. |
E | A1 in the chilled flow top region. |
F | B2 |
Question 45 |
A | Metallic portion of the matrix |
B | Chondrules |
C | CAI’s |
D | Matrix |
E | Nebula |
Question 46 |
A | ...repeated evaporation and condensation. |
B | ...high condensation temperature. |
C | ...high abundance in refractory elements. |
D | ...high abundance in volatile elements. |
Question 47 |
A | Majority of food production ("farming") occur in cratonic regions. |
B | Majority of precious metals were found in cratons. |
C | Majority of oil reserves were found in cratons. |
D | Majority of the diamond-bearing kimberlites were found in cratons. |
Question 48 |
A | 4500 - 4560 |
B | 2500 - 4030 |
C | 542 - 2000 |
D | 3020 - 5560 |
Question 49 |
A | Nd |
B | U |
C | Sm |
D | Th |
E | Pb |
Question 50 |
A | Paleoarchean |
B | Neoarchean |
C | Eoarchean |
D | Mesoarchean |
← |
List |
→ |
1 | 2 | 3 | 4 | 5 |
6 | 7 | 8 | 9 | 10 |
11 | 12 | 13 | 14 | 15 |
16 | 17 | 18 | 19 | 20 |
21 | 22 | 23 | 24 | 25 |
26 | 27 | 28 | 29 | 30 |
31 | 32 | 33 | 34 | 35 |
36 | 37 | 38 | 39 | 40 |
41 | 42 | 43 | 44 | 45 |
46 | 47 | 48 | 49 | 50 |
End |
Credits: Based on the excellent class notes provided by, Dr. Rajeev Nair during Fall 2014.
FAQ | Report an Error
You may download this exam as a PDF file here.
If you get a question wrong, you can still click on the other answers. This will open up hints and explanations (if available), which will provide additional information.
This class covers rapidly evolving subject matter. Due to cutting-edge research into Early Earth, there is a very high possibility that some of the questions may not be relevant to your current understanding. Please use this quiz with caution.