Thursday, February 28, 2013

Douglas Middendorf Quiz

Why is Earth geologically active?
Earth is geologically active because of its Internal heat.
What processes shape Earth's surface?
Impact cratering, volcanism, tectonics, and erosion.
How does Earth's atmosphere affect the planet?
Earths atmosphere shields us from solar radiation and makes the green house effect possible.
Was there ever geological activity on the Moon or Mercury?
Both had volcanism and tectonics but are now geologically dead because of their small size.
Who was Evangelista Torricelli?
An Italian physicist and mathematician, known for his barometer.
What is plate tectonics?
A theory explaining the structure of the earth's crust and many associated phenomena as resulting from the interaction of rigid lithospheric plates that move slowly over the underlying mantle
Is there heat inside Earth?
Yes.
What is convection?
The movement caused within a fluid by the tendency of hotter and therefore less dense material to rise, and colder, denser material to sink under the influence of gravity, which consequently results in transfer of heat
What is conduction?
The process by which heat or electricity is directly transmitted through a substance whenthere is a difference of temperature or of electrical potential between adjoining regions, without movement of the material
What is  radiation?
The emission of energy as electromagnetic waves or as moving subatomic particles.

Quiz


  1. What geological features tell us that water once flowed on Mars?
  2. Why did Mars change?
  3. Is Venus geologically active?
  4. Why is Venus so hot?
  5. What unique features of Earth are important for life?
  6. How is human activity changing our planet?
  7. What makes a planet habitable?
  8. Was there a volcano born last century on Earth?
  9. Which country witnessed a new volcano on February 20, 1943?
  10. Who was working on the field when the volcano was born?
Hint: Use Wikipedia (Paricutin)

U.S. Cities on Front Line as Sea Levels Rise: Scientific American

U.S. Cities on Front Line as Sea Levels Rise: Scientific American:

 "The signs of rising water are everywhere in this seaport city: yellow "Streets May Flood" notices are common at highway underpasses, in low-lying neighborhoods and along the sprawling waterfront."

'via Blog this'

Paricutín: “Save Me From the Dangers in Which I am About to Die” | Rosetta Stones, Scientific American Blog Network

Paricutín: “Save Me From the Dangers in Which I am About to Die” | Rosetta Stones, Scientific American Blog Network:

"Dionisio Pulido suddenly found himself having a very bad day."

'via Blog this'

Chapter 7 notes con't


Outgassing
            Volcanism also a release gas from earth’s interior onto the atmosphere.
Convection of the mantle creates stresses in the crust called tectonic forces.
Compression forces make mountain ranges.
A valley can form where the crust is pulled apart.
Erosion is a blanket term for weather driven processes that break down or transport rock.
Processes that cause erosion include
            Glaciers
            Rivers
            Wind
Erosion can create new features by depositing debris.


Effects of atmosphere on earth
            Erosion
            Radiation protection:
                        All x-ray light is absorbed very high in the atmosphere.
                        Ultraviolet light is absorbed by ozone.
                        Earth’s atmosphere absorbs light at most wavelengths.
            Greenhouse effect
                        Any gas that absorbs infrared
                        Greenhouse gas- molecules with two different types of elements
                        Not a greenhouse gas- molecules with one or two atoms of the same element.
                        Because of the greenhouse effect, earth is much warmer.
            Makes the sky blue!
Atmosphere scatters blue light from the sun, making it appear to come from different directions
                        Sunsets are red because less of the red light from the sun is scattered.
Tectonics
            Long cliffs indicate that Mercury shrank early in its history.
Mars versus Earth
            50 percent earth’s radius, 10 percent Earth’s mass
            1.5 AU from the sun
            Axis tilt about the same as earth
            Similar rotation period
            Thin CO2 atmosphere: little greenhouse
            Main difference: mars is SMALLER   
Seasons on mars are more extreme in the southern hemisphere because of its elliptical orbit.
Seasonal winds on Mars can drive huge dust storms
The surface of Mars appears to have ancient riverbeds
Magnetic field may have preserved early Martian atmosphere.
Solar wind may have stripped atmosphere after field decreased because of interior cooling.
Cratering on Venus
            Impact craters but fewer than the moon, mercury, and mars.
            Many volcanoes
            Fractured and contorted surface indicates tectonic stresses.
Most of earths major geological features can be attributed to plate tectonics, which gradually remakes earths surfaces.
Venus does not appear to have plate tectonics.
Venus is so hot because of a runaway greenhouse effect.
Venus has a very thick carbon dioxide atmosphere with a surface pressure 90 times that of earth.
Thick carbon dioxide atmosphere produces an extremely strong greenhouse effect.
Reflective clouds contain droplets of sulfuric acid.
The runaway greenhouse effect would account for why Venus has little water.
Idea of continental drift was inspired by puzzle like fit of continents.
Mantle material erupts where seafloor spreads.
Changes in earth’s axis tilt might lead to ice ages.
Widespread ice tends to lower global temps by increasing earths reflectivity.
Human activity is driving many other species to extinction.
Human use of fossil fuels produces greenhouse gases that lead to global warming.
Located at an optimal distance from the sun for liquid water to exist.

Wednesday, February 27, 2013

QUIZ 11


Vinnie Caringella           
Astronomy
2-27
Quiz11
1.     Earth retains plenty of internal heat because it is large for a terrestrial planet, the circulation of molten metal in the core generates Earths magnetic field.
2.     Impact cratering, volcanism, tectonics, and erosion
3.     Erosion, Protection from radiation. Greenhouse effect
4.     Cratering shows that the activity ceased long ago
5.     Evangelista Torricelli was an Italian physicist and mathematician, best known for his invention of the barometer.
6.     Scientific theory that describes the large-scale motions of Earth's lithosphere.
7.     YES
8.     Convection is a mode of heat transfer, which includes the movement of the molecules of the material. It is only observed in liquids and gases. It is not possible in solids because the molecules in solids are tightly packed and are not free to move.
9.    
In thermal conduction, thermal energy (heat) transfers through a substance from a hotter region toward a cooler region. For example, when you dip a metal spoon into a cup of tea, the heat from the hot tea will conduct along the spoon so that the handle becomes warm, even though the handle is not in direct contact with the hot tea.
      In electrical conduction, free electrons pass through a substance, thus enabling an electric current.

10.The emission of energy as electromagnetic waves or as moving subatomic particles.



Doug Middendorf Quiz

How do we detect planets around other stars?
Direct Observation, astrometry, doppler shift, pulsar timing, gravitational microlensing and brightness variations.
How do extrasolar planets compare with planets in our solar system
Most of the detected planets have orbits smaller than Jupiter’s, and have a greater mass.
Do we need to modify our theory of solar system formation?
Nebular theory predicts that massive Jupiter-like planets should not form inside the frost line (at << 5 AU). The discovery of “hot Jupiters” has forced a reexamination of nebular theory. 
What is a Hot Jupiter? 
Massive planets that orbit very close to their stars.
Do extrasolar systems have a frost line?
Yes.
Define the frost line
The distance from a star where it is cool enough for hydrogen compounds to solidify.
On which side of the frost line is Earth?
The Earth lies less than a quarter of the distance to the frost line.
On which side of the frost line is Jupiter?
In between Jupiter and Mars' orbits.
What is a meteorite?
An asteroid or comet that has reached earth from outer space. 
What hit Russia last Friday, February 15, 2013? 
A meteorite.

Tuesday, February 26, 2013

Quiz


  1. Why is Earth geologically active?
  2. What processes shape Earth's surface?
  3. How does Earth's atmosphere affect the planet?
  4. Was there ever geological activity on the Moon or Mercury?
  5. Who was Evangelista Torricelli?
  6. What is plate tectonics?
  7. Is there heat inside Earth?
  8. What is convection?
  9. What is conduction?
  10. What is  radiation?
Hint: Use Wikipedia

Chapter 7 Notes


Mercury- craters, smooth plains and cliffs. Closest planet to the sun.
Venus- volcanoes and few craters.
Moon- craters and smooth plains.
Earth is the only planet to have water on its surface.
Earth:
            Core: highest density; nickel and iron
            Mantle: moderate density; silicon and oxygen
            Crust: lowest density; granite and basalt
Gravity pulls high-density material to center.
Lower-density material rises to surface.
Material ends up separated by density.
A planets’ outer layer of cool, rigid rock is call the lithosphere.
It floats on the warmer softer rock that lies beneath.
Rock stretches when pulled slowly but breaks when pulled rapidly.
The gravity of a large world pulls slowly on its rocky content, shaping the world into a sphere.
Heat drives geological activity:
            Convection: hot rock rises, cool rock falls.
            One convection cycle takes 100 million years on earth.
Sources of internal heat
            Gravitational potential energy of accreting planetesimals.
            Differentiation
            Radioactivity
Cooling of interior
            Convection: transports heat as hot material rises and cool material
            Conduction: transfers heat from hot material to cool material.
            Radiation: sends energy into space.

Role of size
            Smaller worlds cool off faster and harden earlier.
            The moon and mercury are now geologically “dead”.
Surface area-to-volume ratio
            Heat content depends on volume.
            Loss of heat through radiation depends on surface area.
            Time to cool depends on surface area divided by volume.
            Larger objects have a smaller ratio and cool more slowly.
Impact cratering
            Impacts by asteroids or comets
Volcanism
            Eruption of molten rock onto surface
Tectonics
            Disruption of a planet’s surface by internal stresses.
Erosion
            Surface changes made by wind water, or ice.

Megan DeCianni Quiz


How do extrasolar planets compare with planets in our solar system?
Most extrasolar planets are jovian planets that are larger than Jupiter. They also have different orbital characteristics than in our solar system

How do we detect planets around other stars?
Directly and indirectly

What is a Hot Jupiter? 
Has a Jupiter-like mass but a much higher surface temperature

Do we need to modify our theory of solar system formation?
No, more than a decade of re-examination haven't discovered any flaws in basic theory
Define the frost line
The minimum distance at which is cold enough for ice to condense.

Do extrasolar systems have a frost line?
Yes
On which side of the frost line is Jupiter?
In between Jupiter and Mars' orbits

On which side of the frost line is Earth?
Earth lies less than 1/4 of the distance to the frost line

What is a meteorite?
A mass of stone, rock, or metal from outer space

What hit Russia last Friday, February 15, 2013? 
A meteorite

Monday, February 25, 2013

Edward O. Wilson


The task of understanding humanity is too important and too daunting to leave to the humanities. Their many branches, from philosophy to law to history and the creative arts, have described the particularities of human nature with genius and exquisite detail, back and forth in endless permutations. But they have not explained why we possess our special nature and not some other out of a vast number of conceivable possibilities. In that sense, the humanities have not accounted for a full understanding of our species’ existence.
So, just what are we? The key to the great riddle lies in the circumstance and process that created our species. The human condition is a product of history, not just the six millenniums of civilization but very much further back, across hundreds of millenniums. The whole of it, biological and cultural evolution, in seamless unity, must be explored for an answer to the mystery. When thus viewed across its entire traverse, the history of humanity also becomes the key to learning how and why our species survived.
A majority of people prefer to interpret history as the unfolding of a supernatural design, to whose author we owe obedience. But that comforting interpretation has grown less supportable as knowledge of the real world has expanded. Scientific knowledge (measured by numbers of scientists and scientific journals) in particular has been doubling every 10 to 20 years for over a century. In traditional explanations of the past, religious creation stories have been blended with the humanities to attribute meaning to our species’s existence. It is time to consider what science might give to the humanities and the humanities to science in a common search for a more solidly grounded answer to the great riddle.
To begin, biologists have found that the biological origin of advanced social behavior in humans was similar to that occurring elsewhere in the animal kingdom. Using comparative studies of thousands of animal species, from insects to mammals, they have concluded that the most complex societies have arisen through eusociality — roughly, “true” social condition. The members of a eusocial group cooperatively rear the young across multiple generations. They also divide labor through the surrender by some members of at least some of their personal reproduction in a way that increases the “reproductive success” (lifetime reproduction) of other members.
Leif Parsons
Eusociality stands out as an oddity in a couple of ways. One is its extreme rarity. Out of hundreds of thousands of evolving lines of animals on the land during the past 400 million years, the condition, so far as we can determine, has arisen only about two dozen times. This is likely to be an underestimate, due to sampling error. Nevertheless, we can be certain that the number of originations was very small.
Furthermore, the known eusocial species arose very late in the history of life. It appears to have occurred not at all during the great Paleozoic diversification of insects, 350 to 250 million years before the present, during which the variety of insects approached that of today. Nor is there as yet any evidence of eusocial species during the Mesozoic Era until the appearance of the earliest termites and ants between 200 and 150 million years ago. Humans at the Homo level appeared only very recently, following tens of millions of years of evolution among the primates.
Once attained, advanced social behavior at the eusocial grade has proved a major ecological success. Of the two dozen independent lines, just two within the insects — ants and termites — globally dominate invertebrates on the land. Although they are represented by fewer than 20 thousand of the million known living insect species, ants and termites compose more than half of the world’s insect body weight.
The history of eusociality raises a question: given the enormous advantage it confers, why was this advanced form of social behavior so rare and long delayed? The answer appears to be the special sequence of preliminary evolutionary changes that must occur before the final step to eusociality can be taken. In all of the eusocial species analyzed to date, the final step before eusociality is the construction of a protected nest, from which foraging trips begin and within which the young are raised to maturity. The original nest builders can be a lone female, a mated pair, or a small and weakly organized group. When this final preliminary step is attained, all that is needed to create a eusocial colony is for the parents and offspring to stay at the nest and cooperate in raising additional generations of young. Such primitive assemblages then divide easily into risk-prone foragers and risk-averse parents and nurses.
Leif Parsons
What brought one primate line to the rare level of eusociality? Paleontologists have found that the circumstances were humble. In Africa about two million years ago, one species of the primarily vegetarian australopithecine evidently shifted its diet to include a much higher reliance on meat. For a group to harvest such a high-energy, widely dispersed source of food, it did not pay to roam about as a loosely organized pack of adults and young like present-day chimpanzees and bonobos. It was more efficient to occupy a campsite (thus, the nest) and send out hunters who could bring home meat, either killed or scavenged, to share with others. In exchange, the hunters received protection of the campsite and their own young offspring kept there.
From studies of modern humans, including hunter-gatherers, whose lives tell us so much about human origins, social psychologists have deduced the mental growth that began with hunting and campsites. A premium was placed on personal relationships geared to both competition and cooperation among the members. The process was ceaselessly dynamic and demanding. It far exceeded in intensity anything similar experienced by the roaming, loosely organized bands of most animal societies. It required a memory good enough to assess the intentions of fellow members, to predict their responses, from one moment to the next; and it resulted in the ability to invent and inwardly rehearse competing scenarios of future interactions.
The social intelligence of the campsite-anchored prehumans evolved as a kind of non-stop game of chess. Today, at the terminus of this evolutionary process, our immense memory banks are smoothly activated across the past, present, and future. They allow us to evaluate the prospects and consequences variously of alliances, bonding, sexual contact, rivalries, domination, deception, loyalty and betrayal. We instinctively delight in the telling of countless stories about others as players upon the inner stage. The best of it is expressed in the creative arts, political theory, and other higher-level activities we have come to call the humanities.
The definitive part of the long creation story evidently began with the primitive Homo habilis (or a species closely related to it) two million years ago. Prior to the habilines the prehumans had been animals. Largely vegetarians, they had human-like bodies, but their cranial capacity remained chimpanzee-size, at or below 500 cubic centimeters. Starting with the habiline period the capacity grew precipitously: to 680 cubic centimeters in Homo habilis, 900 in Homo erectus, and about 1,400 in Homo sapiens. The expansion of the human brain was one of the most rapid episodes of evolution of complex organs in the history of life.

Still, to recognize the rare coming together of cooperating primates is not enough to account for the full potential of modern humans that brain capacity provides. Evolutionary biologists have searched for the grandmaster of advanced social evolution, the combination of forces and environmental circumstances that bestowed greater longevity and more successful reproduction on the possession of high social intelligence. At present there are two competing theories of the principal force. The first is kin selection: individuals favor collateral kin (relatives other than offspring) making it easier for altruism to evolve among members of the same group. Altruism in turn engenders complex social organization, and, in the one case that involves big mammals, human-level intelligence.
The second, more recently argued theory (full disclosure: I am one of the modern version’s authors), the grandmaster is multilevel selection. This formulation recognizes two levels at which natural selection operates: individual selection based on competition and cooperation among members of the same group, and group selection, which arises from competition and cooperation between groups. Multilevel selection is gaining in favor among evolutionary biologists because of a recent mathematical proof that kin selection can arise only under special conditions that demonstrably do not exist, and the better fit of multilevel selection to all of the two dozen known animal cases of eusocial evolution.
The roles of both individual and group selection are indelibly stamped (to borrow a phrase from Charles Darwin) upon our social behavior. As expected, we are intensely interested in the minutiae of behavior of those around us. Gossip is a prevailing subject of conversation, everywhere from hunter-gatherer campsites to royal courts. The mind is a kaleidoscopically shifting map of others, each of whom is drawn emotionally in shades of trust, love, hatred, suspicion, admiration, envy and sociability. We are compulsively driven to create and belong to groups, variously nested, overlapping or separate, and large or small. Almost all groups compete with those of similar kind in some manner or other. We tend to think of our own as superior, and we find our identity within them.
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Read previous contributions to this series.
The existence of competition and conflict, the latter often violent, has been a hallmark of societies as far back as archaeological evidence is able to offer. These and other traits we call human nature are so deeply resident in our emotions and habits of thought as to seem just part of some greater nature, like the air we all breathe, and the molecular machinery that drives all of life. But they are not. Instead, they are among the idiosyncratic hereditary traits that define our species.
The major features of the biological origins of our species are coming into focus, and with this clarification the potential of a more fruitful contact between science and the humanities. The convergence between these two great branches of learning will matter hugely when enough people have thought it through. On the science side, genetics, the brain sciences, evolutionary biology, and paleontology will be seen in a different light. Students will be taught prehistory as well as conventional history, the whole presented as the living world’s greatest epic.
We will also, I believe, take a more serious look at our place in nature. Exalted we are indeed, risen to be the mind of the biosphere without a doubt, our spirits capable of awe and ever more breathtaking leaps of imagination. But we are still part of earth’s fauna and flora. We are bound to it by emotion, physiology, and not least, deep history. It is dangerous to think of this planet as a way station to a better world, or continue to convert it into a literal, human-engineered spaceship. Contrary to general opinion, demons and gods do not vie for our allegiance. We are self-made, independent, alone and fragile. Self-understanding is what counts for long-term survival, both for individuals and for the species.

Edward O. Wilson
Edward O. Wilson is Honorary Curator in Entomology and University Research Professor Emeritus, Harvard University. He has received more than 100 awards for his research and writing, including the U. S. National Medal of Science, the Crafoord Prize and two Pulitzer Prizes in non-fiction. His most recent book is “The Social Conquest of Earth.”

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QUIZ - Due on 2.26.13

  1. How do we detect planets around other stars?
    • We can detect planets around other stars with the help of direct observation, astrometry, doppler shift, pulsar timing, brightness variations, and gravitational microlensing.
    • DIRECTLY: Pictures or spectra of the planets themselves constitute direct evidence of their existence.
    • INDIRECTLY: Precise measurements of a star's properties may indirectly reveal the effects of orbiting planets. (Almost all extrasolar planets detected to date have been found indirectly rather than through direct imagine.)
      • Orbiting planets exert gravitational tugs on their star, so we can detect the planets by observing the stars resulting "wobble" around its average position in the sky.
  • How do extrasolar planets compare with planets in our solar system?
    • Extrasolar planets compare with planets in our solar system becuase most known extrasolar planets are probably jovian. We've also found "Super Earths," likely made of metal and rock.
      • Extrasolar planets (most) are more massive than Jupiter.
      • Extrasolar planets (most) have different orbital characteristics than in our solar system.
      • Detected planets are all way more massive than Earth.
  • Do we need to modify our theory of solar system formation?
    • At this moment in time, we do not need to modify our theory of solar system formation. Our current theory has presented challenges, but more than a decade of re-examination hasn't resulted in any obvious flaws. In the future, the basic theory encounters & migration may play a larger role than previously thought.
  • What is a Hot Jupiter?
    • Hot Jupiter is a class of extrasolar planets who characteristics are similar to Jupiter. They have a much higher surface temperatures because they orbit very close between approximately 0.015 & 0.5 astronimical units to their parent star.
  • Do extrasolar systems have a frost line?
    • YES!
  • Define the frost line.
    • Front line is a particular distance in the solar nebula from the central protosun where it is cool enough for hydrogen compounds such as water, ammonia, and methane to condense into solid ice grains.
  • On which side of the frost line is Earth?
    • The Earth lies < than 1/4 of the distance to the frost line.
  • On which side of the frost line is Jupiter?
    • In between Jupiter and Mars' orbits lies the Frost Lines.
  • What is a meteorite?
    • A meteorite is a mass of stone, rock, or metal from outer space: a piece of rock that has reached Earth from outer space.
  • What hit Russia last Friday, February 15, 2013?
    • On Friday, February 15th, 2013 a meteorite / meteoride hit Russia.