20180501

Online reading assignment: Milky Way history, big bang clues (NC campus)

Astronomy 210, spring semester 2018
Cuesta College, San Luis Obispo, CA

Students have a weekly online reading assignment (hosted by SurveyMonkey.com), where they answer questions based on reading their textbook, material covered in previous lectures, opinion questions, and/or asking (anonymous) questions or making (anonymous) comments. Full credit is given for completing the online reading assignment before next week's lecture, regardless if whether their answers are correct/incorrect. Selected results/questions/comments are addressed by the instructor at the start of the following lecture.

The following questions were asked on reading textbook chapters and previewing presentations on the history of the Milky Way and big bang clues, a comic strip adaptation of of Neil deGrasse Tyson's "The Most Astounding Fact" 2008 interview for TIME magazine, and Minute Physics' video explanation of Olbers' paradox.


Selected/edited responses are given below.

Describe something you found interesting from the assigned textbook reading or presentation preview, and explain why this was personally interesting for you.
"How dirty space actually is."

"How metals were produced by a type II supernovas, because I never would have guessed that metals goes back that far."

"How we are able to detect metals in stars. Astronomy is just interesting all together."

"How our bodies originated from starstuff because you always see those Facebook posts that say that you are made from starstuff and never really understand them."

"That the halo of the Milky Way has older stars than the disk."

"Lookback time is very interesting because it’s so confusing, it's intriguing to think about."

"The big bang, because honestly, that seems to be the extent of knowledge that man kind can have, because its impossible to know what occurred before then. "

"The big bang, because it was the start of the universe and life itself. I find it interesting how at some point there was nothing and then spontaneously, there was something that started everything in the galaxy and there is no true answer as to how it all started."

Describe something you found confusing from the assigned textbook reading or presentation preview, and explain why this was personally confusing for you.
"How some stars are more metal-rich than others."

"Why older stars are metal-poor and newer ones are metal-rich."

"Let me get this straight, older stars (first generation) are metal-poor? I thought stars fuse hydrogen into heavier elements...so older ones would have more metal... I'm definitely confused."

"Why the sky is dark at night, because it the video that we watched did not seem to give a definite answer as to the reason actually why the night sky is dark, but reasons as to why the night sky isn't bright from other stars."

"Lookback time, because I didn't realize we are looking in the past at these other galaxies."

"The big bang is sort of confusing to me because I'm still not completely sure what it exactly was caused by or made up of and how it can create a massive universe."

"I don't understand how we can really gauge if there are edges on the universe. And would would be past the edge?"

"How the universe is always expanding."

"Again, the big bang, because the concept as a whole is mind boggling, there is a physical point that scientifically we can't go further back then. But the universe has always existed, what started it? Can nothingness condense into matter? It's weird."

Indicate how the amount of these elements in the universe have changed over time.
(Only correct responses shown.)
Hydrogen: decreased [56%]
Metals (elements heavier than hydrogen and helium): increased [69%]

The outermost layers of __________ are more abundant in metals (elements heavier than hydrogen and helium).
extremely old stars that formed a long time ago.  **** [4]
young stars that formed very recently.  ********** [10]
(There is a tie.)  [0]
(Neither, as stars cannot have metals.)  [0]
(Unsure/guessing/lost/help!)  ** [2]

Indicate what produced these elements.
(Only correct responses shown.)
Hydrogen in the sun's core: the very early universe [63%]
Helium in the sun's core: the sun [75%]
Carbon in your body: another star, in the past [63%]
Calcium in your bones: another star, in the past [50%]
Iron in your blood: another star, in the past [56%]
Gold and silver from mines: another star, in the past [50%]

Ask the instructor an anonymous question, or make a comment. Selected questions/comments may be discussed in class.
"Just need clarification on what elements of the sun and the universe produced."

"'It turns out that we have a time-machine of sorts to actually see the universe as it was in the past... This means that when we look at Deneb in the night sky tonight (season permitting), we are seeing Deneb not as it is now, but as it was in the past, 1,400 years ago.' I love this so much. This just rocks my world."

"I've been working on my research project since I got home and I AM SO PROUD OF MYSELF I feel like I finally understand galaxies. Well you're going to see my whole project Fri-yay and be like yeeeeaaah I KNEW those would be your results because I understand the greater meaning of life itself. Just kidding, you don't sound like that. ANYWAYS my conclusion is like 5 paragraphs because I keep making connections with all the other stuff we've learned like OF COURSE MOST SPIRAL GALAXIES ARE BLUE OR WHITE BECAUSE THEY ARE COMPRISED MOSTLY OF GAS AND DUST WHICH IS BREEDING GROUNDS FOR BABY STARS AND THERE ARE PRACTICALLY NO RED OR ORANGE ONES BECAUSE ELLIPTICAL GALAXIES ARE THE HOME FOR OLD FARTY STARS/GALAXIES. My research conclusion actually uses science terminology so don't worry I won't call them farty, but I know you'll know what I mean. ANYWAYS that's why I haven't done the reading for these chapters because I'm a poop and a procrastinator BUT I am making leaps on my research thingie-ma-bobbie. PS yes that is a technical term and I WILL be using it on my project board...I lied, it won't be on my board. I need sleep. Do you feel accomplished when students are finally able to connect work from one subject to another? Assuming your answer is yes because, well if you didn't you probably wouldn't care about our grades or us. WHICH I think you do. hopefully I pass this class and not just the dang lab."

"Why does the universe keep expanding does it ever stop growing?"

"What is your favorite topic to teach in astronomy?" (Pretty much this week's topics--our place in the universe and how we understand how we got here. But then there was everything else about the stars and the Milky Way that we need to learn just go get to this point in the semester. So pretty everything.)

"Is the class over after the final?" (Uh, yes? Well, hopefully not really, and you'll still be learning about astronomy even after the end of the semester.)

"Since I am doing well in the class... May an I get an 'A' for the class now, and not be required to take the final exam?" (You're so close--so if you can get there on your own before finals week, then yes, you wouldn't need more points from the Final Exam.)

"You must be happy that summer is approaching! (Yes. This is me looking forward to summer.)

20180430

Online reading assignment: Feynman diagram vertices

Physics 205B, spring semester 2018
Cuesta College, San Luis Obispo, CA

Students have a weekly online reading assignment (hosted by SurveyMonkey.com), where they answer questions based on reading their textbook, material covered in previous lectures, opinion questions, and/or asking (anonymous) questions or making (anonymous) comments. Full credit is given for completing the online reading assignment before next week's lecture, regardless if whether their answers are correct/incorrect. Selected results/questions/comments are addressed by the instructor at the start of the following lecture.

The following questions were asked on reading presentations Feynman diagrams (Phillip "Flip" Tanedo, Cornell University/USLHC Collaboration) and quantum electrodynamics (QED) (Christopher "Bot" Skilbeck, cronodon.com).

The Big Bang Theory (Pilot)
Warner Bros. Television (2007)
bigbangtheory.wikia.com/wiki/User_blog:Sheldon_Cooper_PhD/Pilot

Selected/edited responses are given below.

Describe what you understand from the assigned textbook reading or presentation preview. Your description (2-3 sentences) should specifically demonstrate your level of understanding.
"Feynman diagrams are used to describe the interactions between electrons and positrons. The interactions of electrons and positrons can resulting in absorbing a photon, emitting a photon, or a electron being annihilated by a positron."

"Lines in these diagrams represent particles. Every particle has to meet at an intersection that is called an interaction. You can't have a vertex with only squiggly lines (photons) with no particle lines flowing into or out from it."

"Feynman diagrams are how we can visualize particle physics, specifically the interactions of electrons, positrons, and photons. We read the diagrams left-to-right, as they are a representation of what happens over a certain amount of time."

"The Feynman diagrams are meant to indicate the path that the particles take through space. We interpret the x-axis as the direction of time and the y-axis as the space direction."

"A left-to-right arrow is an electron, the opposite is a positron and a wiggly line is a photon. the rest is very vague and I need more explanations on various cases and what they mean."

"Positrons point to the left, electrons point to the right. Gamma (squiggly line) are photons. A Feynman diagram should only contain connected pieces, and any diagram with arrows going into a gamma needs arrows coming out or else it isn't an accurate diagram."

"Honestly, there wasn't much I understood."

Describe what you found confusing from the assigned textbook reading or presentation preview. Your description (2-3 sentences) should specifically identify the concept(s) that you do not understand.
"Everything. I don't get Feynman diagrams."

"Why do we use Feynman diagrams? They just seem like squiggles a 3 year-old could draw, why is there not another way to represent these forces interacting?"

"Is an electron moving in the opposite direction a positron? What actually is a positron?"

"All good so far."

"Specifically how the diagrams are to be used."

"I don't think I would really be able to interpret them on my own. It would be helpful to do this in class."

"This is all pretty trippy. I want to learn more about what diagrams are possible and which are not."

When reading Feynman diagrams, time runs from:
bottom to top.  [0]
top to bottom.  ** [2]
left to right.  ******************* [19]
right to left.  * [1]
(Unsure/guessing/lost/help!)  **** [4]

Describe how the path of an electron and the path of a positron are drawn differently on a Feynman diagram. (Note that both paths have the same "e" labels.)
"Electrons point right and positrons point to the left."

"A position is indicated as e+ therefore, the electron will always be drawn traveling from right to left. Meanwhile, an electron is indicated by an e- and will always be drawn traveling left to right. This way, when they are being read, we can see that the arrows are point in the direction of the flow of electron charge."

"Positrons (antimatter) point to the left, electrons point to the right."

Describe what will happen if an electron meets a positron.
"Annihilation will happen."

"They will cancel each other out and create pure energy."

"They make a big bang!"

"It becomes something else (the other symbol thing)?"

The above (valid) Feynman diagram depicts an electron:
absorbing a photon.  *** [3]
emitting a photon.  ******************* [19]
annihilated by a positron.  * [1]
(Unsure/guessing/lost/help!)  *** [3]

The above (valid) Feynman diagram depicts an electron:
absorbing a photon.  *** [3]
emitting a photon.  ***** [5]
annihilated by a positron.  ************** [14]
(Unsure/guessing/lost/help!)  **** [4]

The above (valid) Feynman diagram depicts an electron:
absorbing a photon.  ***************** [17]
emitting a photon.  * [1]
annihilated by a positron.  **** [4]
(Unsure/guessing/lost/help!)  **** [4]

Explain why the above Feynman diagram is invalid.
"Two arrows are going into the vertex. One needs to be going out."

"The two electrons cannot intersect at the same point how this one is depicted."

"The two electrons cannot crash like that."

Ask the instructor an anonymous question, or make a comment. Selected questions/comments may be discussed in class.
"What are all these squiggles and arrows about?"

"A very basic lecture on what every symbol is called and what happens when they mix would be of great benefit."

"My mind is blown.:

20180429

Astronomy current events question: Mars Express software upgrade

Astronomy 210L, spring semester 2018
Cuesta College, San Luis Obispo, CA

Students are assigned to read online articles on current astronomy events, and take a short current events quiz during the first 10 minutes of lab. (This motivates students to show up promptly to lab, as the time cut-off for the quiz is strictly enforced!)
News release, "Mars Express 2.0" (April 11, 2018)
esa.int/Our_Activities/Operations/Mars_Express_v2.0
The European Space Agency's Mars Express spacecraft will undergo a software upgrade to:
(A) reformat memory.
(B) increase photo resolution.
(C) conserve battery power.
(D) fully extend its solar panels.
(E) reduce gyroscope wear.

Correct answer: (E)

Student responses
Sections 30679, 30680
(A) : 4 students
(B) : 6 students
(C) : 4 students
(D) : 1 student
(E) : 19 students

Astronomy current events question: CubeSat ASTERIA test

Astronomy 210L, spring semester 2018
Cuesta College, San Luis Obispo, CA

Students are assigned to read online articles on current astronomy events, and take a short current events quiz during the first 10 minutes of lab. (This motivates students to show up promptly to lab, as the time cut-off for the quiz is strictly enforced!)
Calla Cofield, "Astrophysics CubeSat Demonstrates Big Potential in a Small Package" (April 12, 2018)
jpl.nasa.gov/news/news.php?feature=7097
The Arcsecond Space Telescope Enabling Research in Astrophysics (ASTERIA) satellite recently proved low-cost spacecraft can steadily monitor a star's brightness to search for:
(A) solar flares.
(B) parallax.
(C) repeating nova explosions.
(D) Doppler shifts.
(E) orbiting exoplanets.

Correct answer: (E)

Student responses
Sections 30679, 30680
(A) : 4 students
(B) : 2 students
(C) : 4 students
(D) : 0 students
(E) : 24 students

Astronomy current events question: "Ultima Thule"

Astronomy 210L, spring semester 2018
Cuesta College, San Luis Obispo, CA

Students are assigned to read online articles on current astronomy events, and take a short current events quiz during the first 10 minutes of lab. (This motivates students to show up promptly to lab, as the time cut-off for the quiz is strictly enforced!)
Tricia Talbert, "New Horizons Chooses Nickname for 'Ultimate' Flyby Target" (March 13, 2018)
nasa.gov/feature/new-horizons-chooses-nickname-for-ultimate-flyby-target
NASA's New Horizons spacecraft will visit (486958) 2014 MU69, nicknamed "Ultima Thule," which means:
(A) "Eternal Twilight."
(B) "Final Destination."
(C) "King Thule's Last Voyage."
(D) "Beyond the Northernmost Island."
(E) "Ancient Forest of Darkness."

Correct answer: (B)

Student responses
Sections 30679, 30680
(A) : 4 students
(B) : 7 students
(C) : 3 students
(D) : 20 students
(E) : 0 students

20180425

Online reading assignment: radioactive decay modes

Physics 205B, spring semester 2018
Cuesta College, San Luis Obispo, CA

Students have a weekly online reading assignment (hosted by SurveyMonkey.com), where they answer questions based on reading their textbook, material covered in previous lectures, opinion questions, and/or asking (anonymous) questions or making (anonymous) comments. Full credit is given for completing the online reading assignment before next week's lecture, regardless if whether their answers are correct/incorrect. Selected results/questions/comments are addressed by the instructor at the start of the following lecture.

The following questions were asked on reading textbook chapters and previewing presentations on radioactive decay modes.


Selected/edited responses are given below.

Describe what you understand from the assigned textbook reading or presentation preview. Your description (2-3 sentences) should specifically demonstrate your level of understanding.
"The atomic number represents the total amount of protons. The nucleon number represents the combined number of protons and neutrons. The number of neutrons can be determined by having the nucleon number minus the atomic number."

"The different decays all achieve stability through different means. Some expel particles while other transform particles into other ones."

"The key to stability is being able to keep the protons in the nucleus together. Alpha decay is how a nucleus with excess protons achieves a more stable configuration. Beta-minus decay is how a nucleus with excess neutrons achieves a more stable configuration. Beta-plus decay is how a nucleus that is neutron deficient achieves a more stable configuration. Gamma decay is how a nucleus achieves a more stable configuration, but not because it has too many protons, or the wrong ratio of protons to neutrons."

"For all atomic nuclei the key to stability is being able to keep the protons in the nucleus together. Also, having a certain number of neutrons in the nucleus will decrease the proton-proton repulsion."

"For all atomic nuclei, to have stability they have to keep the protons in the nucleus together, in spite of them all repelling each other. They need to have the proper ratio of neutrons, approximately equal to or slightly greater than the number of protons. More than 83 protons would automatically make the nucleus unstable."

"Stability conditions. A nucleus with more than 83 protons will always be unstable. Neutrons help to balance out proton to proton repulsion so it's necessary to have more neutrons than protons in a nucleus in order to be stabilized. The different decay processes we are learning about are used by nuclei to help them reach stable conditions depending on what makes them unstable to begin with."

"Radioactive decay occurs in four ways. If a nucleus has more than 83 protons, it will emit He to decrease p and n equally (alpha particles). If protons are significantly less than neutrons, neutrons will be converted to protons, releasing antineutrinos and electrons (Β particles). If protons are more numerous than neutrons, protons will be converted to neutrons, releasing positrons (Β+ particles) and neutrinos. Nuclei become excited after decay and will release photons to 'calm down' (gamma particles)."

"This is pretty basic chemistry stuff, it doesn't seem to be a problem."

Describe what you found confusing from the assigned textbook reading or presentation preview. Your description (2-3 sentences) should specifically identify the concept(s) that you do not understand.
"The different types of decay--from a problem-solving perspective it would just be nice to see some different examples going through how to sort each type of decay."

"Most of this was a good refresher on decay and specifically all of the types of it that I learned in the tail-end of my general chemistry series last year."

"I don't understand the difference between a nucleus that is stable or unstable."

"Electron capture and the 'swallowing' thing. And also a bit of gamma decay."

"I like radioactive decay."

"I am having a harder time with gamma (γ) decay. I will do more research to clarify the topic but for right now I'm not grasping it."

"I feel like electron capture was passed over too quickly, I don't really understand what happens."

"What is a neutrino and can it be positive or negative?"

"Outside of confusing the different decay processes this is thankfully review from other classes. "

Explain what a "nucleon number" is, and/or describe how to calculate it for a nucleus.
"It is the total number of protons and neutrons inside the atomic nucleus."

"The nucleon number is the total number of nucleons (protons and electrons), such that the number of neutrons is the difference between the nucleon number and atomic number."

"Not there yet."

Identify the processes that increase, decrease, or do not change the number of protons in the nucleus.
(Only correct responses shown.)
α decay: decrease. [77%]
β– decay: increase. [77%]
β+ decay: decrease. [77%]
electron capture: decrease. [38%]
γ decay: does not change. [69%]

Identify the processes that increase, decrease, or do not change the number of neutrons in the nucleus.
(Only correct responses shown.)
α decay: decrease. [69%]
β– decay: decrease. [65%]
β+ decay: increase. [65%]
electron capture: increase. [19%]
γ decay: does not change. [65%]

Identify the processes that change a proton to a neutron, or change a neutron to a proton in the nucleus.
(Only correct responses shown.)
α decay: no p/n conversion. [62%]
β– decay: n → p. [73%]
β+ decay: p → n. [69%]
electron capture: p → n. [35%]
γ decay: no p/n conversion. [69%]

Ask the instructor an anonymous question, or make a comment. Selected questions/comments may be discussed in class.
"Quiz 6 is going to be awful...I have such a hard time with the right-hand rules and flux laws."

"This seems like it is going to be the most interesting section to date!"

"I think I'll like this chapter a lot better than the previous ones!"

"Could we go over electron capture?"

20180423

Online reading assignment: radioactive decay rates

Physics 205B, spring semester 2018
Cuesta College, San Luis Obispo, CA

Students have a weekly online reading assignment (hosted by SurveyMonkey.com), where they answer questions based on reading their textbook, material covered in previous lectures, opinion questions, and/or asking (anonymous) questions or making (anonymous) comments. Full credit is given for completing the online reading assignment before next week's lecture, regardless if whether their answers are correct/incorrect. Selected results/questions/comments are addressed by the instructor at the start of the following lecture.

The following questions were asked on reading textbook chapters and previewing presentations on radioactive decay rates.


Selected/edited responses are given below.

Describe what you understand from the assigned textbook reading or presentation preview. Your description (2-3 sentences) should specifically demonstrate your level of understanding.
"Exponential and half life decay are both covered well in general chemistry so it's somewhat of a review. But the M&Ms® example is still helpful."

"I understood the introduction to radioactive decay and half-lives. I feel like most of this is from previous biology and chemistry classes."

"Thankfully, this presentation was a bit of a refresher from my other physical science classes. Radioactive dating helps us determine how long the radioactive substance has been around, assuming that there are no daughter atoms to begin with."

"I understand that older substances have more daughter atoms in them. Different elements have different half-lives."

"When there are more daughter atoms the sample is older. The daughter are released when the sample that is being melted, which will then determine the age of the material/sample."

"Radioactive decay can be used to determine the age of an unknown material. This is done using half-lives to measure the time these radioactive materials decay in the unknown material."

"Gaseous daughter atoms can be compared to the amount of radioactive atoms left in a sample to determine how long ago the sample started. After a molten sample solidifies, it will start anew with having radioactive atoms with no daughter atoms."

Describe what you found confusing from the assigned textbook reading or presentation preview. Your description (2-3 sentences) should specifically identify the concept(s) that you do not understand.
"I actually feel okay with this stuff thanks to chemistry and other classes I've taken that have dealt with radioactive decay. Going through the slides one more time will help me understand things more."

"There wasn't anything too confusing from the presentation preview. I have learned about radioactive decay in other classes before."

"I don't understand the equation for half-life decay, or radioactive dating."

"I would like to go over problems to get more familiar with the equations."

"I'm confused with the section on radioactive dating, or carbon dating. How exactly is the age of something determined?"

"I don't understand the process to calculate the half life of a material or why melting an object affects its half-life."

"How is the clock reset when matter is solidified after melting if gaseous daughter particles escape?"

"I am struggling with the melting and solidification ages."

"At the moment I am not sure what I find confusing. Most of the lecture made sense to me as far as I am concerned."

State the SI units for activity (radioactive decays per time).
"Decays/s."

"s–1."

"Bq, or becquerel."

"Curies?"

"Lambda?"

"Not sure."

For a radioactive decay process, the time constant τ ("average lifetime") is __________ half-life T1/2.
less than.  ** [2]
equal to.  ***** [6]
greater than.  ******************* [19]
(Unsure/guessing/lost/help!)  ** [2]

Two samples are each comprised of 800 unstable atoms that will undergo radioactive decay. The remainder of one sample is 200 inert, stable atoms not involved in a radioactive decay process. The remainder of the other sample is 200 daughter atoms of the radioactive decay process.
(Only correct responses shown.)
Sample with more activity (decays/time): (there is a tie). [24%]
Sample with older solidification age: radioactive sample with daughter atoms. [45%]

Describe what changes in a sample when it melted and then solidified that resets its solidification age as determined by radioactive dating.
"Daughter atoms are released and are compared to the radioactive atoms that are left in the sample. Melting it resets its solidification age."

"Since daughter atoms (which are used to date the substance) are gaseous, when the substance is melted they are released. Therefore, they are no longer in the substance effectively resetting the age of the substance."

"There are technically no radioactive atoms or daughter atoms in the sample anymore, so it can reset its solidification age."

"Gaseous daughter atoms are released. This tells us how long ago the sample started with radioactive atoms with no daughter atoms."

"When a substance is liquified the once solidified daughter atoms are released into the air. When the substance is allowed to cool back into a solid the daughter atoms to not solidify back into the original state. This makes its a less reliable in radioactive dating."

"Not sure."

"Hmm..."

Ask the instructor an anonymous question, or make a comment. Selected questions/comments may be discussed in class.
"I really still think I need help with Lenz's law and Faraday's law."

"The semester after spring break is harder than I thought. But I think I will be able to catch up for the final."

"I need to play Half-Life again."

"I'm excited to eat M&Ms®!!!" (Wait for it--we'll get to do this in the last lab.)

20180420

Astronomy current events question: Fast-Evolving Luminous Transient (FELT) explosions

Astronomy 210L, spring semester 2018
Cuesta College, San Luis Obispo, CA

Students are assigned to read online articles on current astronomy events, and take a short current events quiz during the first 10 minutes of lab. (This motivates students to show up promptly to lab, as the time cut-off for the quiz is strictly enforced!)
Ray Villard, Armin Rest, "Kepler Solves Mystery of Fast and Furious Explosions" (March 26, 2018)
http://hubblesite.org/news_release/news/2018-18
NASA's Kepler space telescope's observations of Fast-Evolving Luminous Transient (FELT) explosions may be explained by stars that expel __________ before becoming supernovae.
(A) antimatter.
(B) gas and dust.
(C) dark matter.
(D) neutrinos.
(E) x-ray pulses.

Correct answer: (B)

Student responses
Sections 30679, 30680
(A) : 3 students
(B) : 20 students
(C) : 4 students
(D) : 6 students
(E) : 6 students

Astronomy current events question: volcanic interactions with Mar's oceans?

Astronomy 210L, spring semester 2018
Cuesta College, San Luis Obispo, CA

Students are assigned to read online articles on current astronomy events, and take a short current events quiz during the first 10 minutes of lab. (This motivates students to show up promptly to lab, as the time cut-off for the quiz is strictly enforced!)
Robert Sanders, "Mars' Oceans Formed Early, Possibly Aided by Massive Volcanic Eruptions" (March 20, 2018)
eps.berkeley.edu/news/mars’-oceans-formed-early-possibly-aided-massive-volcanic-eruptions
Researchers propose that Mars' oceans formed much earlier and shallower than previously thought, due to:
(A) volcanic activity.
(B) comet bombardment.
(C) global cooling.
(D) perchlorate rains.
(E) global sandstorms.

Correct answer: (A)

Student responses
Sections 30679, 30680
(A) : 29 students
(B) : 6 students
(C) : 2 students
(D) : 1 student
(E) : 1 student

Astronomy current events question: life in Venus' dark clouds?

Astronomy 210L, spring semester 2018
Cuesta College, San Luis Obispo, CA

Students are assigned to read online articles on current astronomy events, and take a short current events quiz during the first 10 minutes of lab. (This motivates students to show up promptly to lab, as the time cut-off for the quiz is strictly enforced!)
Terry Devitt, "Is There Life Adrift in the Clouds of Venus?" (March 30, 2018)
news.wisc.edu/is-there-life-adrift-in-the-clouds-of-venus/
Researchers propose that dark patches in Venus' atmosphere could be caused by __________ in its clouds.
(A) hydrocarbon hurricanes.
(B) black lightning.
(C) floating microbial life.
(D) sulfuric acid rain.
(E) volcanic outgassing.

Correct answer: (C)

Student responses
Sections 30679, 30680
(A) : 0 students
(B) : 0 students
(C) : 26 students
(D) : 6 students
(E) : 7 students