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