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