EEB Undergraduate Research Symposium Notes

EEB Undergraduate Research Symposium

Event Details

  • Event: EEB Undergraduate Research Symposium
  • Date: Monday, April 28
  • Time: 12:45-5:00 PM
  • Location: Biology/Physics Building, Room 131
  • Refreshments: Light refreshments provided
  • Sponsors: College of Liberal Arts and Sciences, Department of Ecology and Evolutionary Biology

Bonus Activity

  • Worth a maximum of 5 bonus points.
  • Answer the following questions about a newly discovered species.
  • The first letter of the species name must match the first letter of your first name.
    • Example: If your name is Ed, a species named Pizza ellipticum would be acceptable.
Questions
  1. Provide a link to a scientific article describing a new species (discovered between 1975 and the present day).
  2. Where is the species found?
    • Geographic location
    • Habitat
  3. Why had this species avoided detection until now?
  4. What species concept did the researchers use to determine that this was a new species?
    • The article may not explicitly state this.
    • Critically analyze the article and explain why researchers could claim it was a 'new' species rather than a member of a previously described species.

Course Announcements

  • The lowest exam score will be dropped.
  • Final grade calculation:
    • Based on the three highest exam scores (100 points each).
    • Participation activities (maximum 40 points).
    • Any additional bonus points earned.
  • Details available on the course website.

Feathers and Flight

  • Feathers evolved before flight.
Hypotheses for the Initial Evolution of Feathers
  1. Sexual selection
  2. Thermoregulation
  • Reference: Fig. 18.16

Dinosaur Feather Color

  • How was the color of Anchiornis huxleyi feathers determined?
  • Electron microscopy of melanosome structure.
  • Melanosome: “melanin-containing organelles that determine key aspects of color”.
  • Reference: Li et al. 2010 Science.
  • Iridescent dinosaur feathers.
  • A bony-crested Jurassic dinosaur with evidence of iridescent plumage highlights complexity in early paravian evolution.
  • Diameter of melanosomes: 900300900-300 nm, n = 0.1930.193, 0=0.1170 = 0.117
  • Length of melanosomes: 100020001000-2000 nm, n = 0.2310.231, n = 0.2410.241
  • Image credit: Velizar Simeonovski, Field Museum

Evolution of Flight

  • How did flight evolve?
  • Competing hypotheses:
    • Ground up
    • Tree down
  • The exact mechanism is still unknown.
  • Current research focuses on juvenile birds.
  • Reference: Norberg 1990, Vertebrate Flight

Turtle Evolution

  • Transitional fossils clarify turtle evolution
  • Turtles are amniotes like us.
  • Many amniotes have a diagnostic rib development pattern (under the shoulder blades).
  • Turtle shells are formed by rib development going over its shoulder blades.
  • Odontochelys represents an intermediate form that explains turtle relationships with amniotes.
  • Reference: Fig. 2.22

Origin of Mammals

  • There is a well-documented set of fossils showing reptile-like mammals.
  • These fossils allow for evolutionary reconstruction of important mammal-specific traits.
  • Middle ear bones.
  • Reference: Fig. 18.17

Jaw and Middle Ear

  • Mammalian middle ear bones are homologous to jaw bones in relatives.
  • These bones became reduced in size and specialized for hearing.
  • Mammalian jaw evolved a different hinge structure to compensate for these bones being used for hearing.
  • Reference: Fig. 18.18

Taxonomy and Fossils

  • Remember back to species concepts.
  • Which concept applies well to fossils?
  • Morphological and Phylogenetic species concepts can handle fossil data.
  • A major drawback of the Morphological Species Concept (MSC) is not knowing where to draw the line as to what constitutes a new species.

Extinction

  • Way more species have gone extinct than are currently alive.
  • A few intervals of time have a disproportionate amount of extinctions
  • Mass extinctions.
  • Reference: Fig. 18.25
  • Mass extinctions removed many families.
  • Reference: Fig. 18.26
  • Background extinction includes all the extinctions that were happening outside of mass extinction events.
  • Reference: Fig. 18.25
  • Lineages vary in their extinction rates over time.
  • Reference: Fig. 18.27

Causes of Mass Extinctions

  • Depends on the extinction event.
  • The Cretaceous-Paleogene (K-Pg) extinction is highly studied.
  • How do we know the timing of this extinction?
  • In-class activity.
  • Reference: Fig. 18.26

Iridium and Extinction Timing

  • Iridium is rare on Earth but common in space.
  • As researchers dug further into the crust, they encountered increased concentrations of iridium.
  • The inference is that this iridium spike came from space.
  • Back-of-the-envelope calculations suggest that an asteroid the size of a mountain hit Earth.
  • Reference: Fig. 18.29b

Geological Formation Changes

  • Limestone layers are visible above and below a quarter coin.
  • The quarter is placed in a strip of sediment made of clay.
  • Limestone is formed from marine invertebrate shells.
  • The asteroid impact killed these lineages; therefore, no limestone formed for some time.
  • Reference: Fig. 18.29a

Asteroid Impact Site

  • Areas in the Caribbean were found to be rich in minerals consistent with high and quick pressure.
  • Magnetic abnormalities in the Yucatán peninsula provided a key clue.
  • Surveys later showed that the impact left a crater 180 km wide near Chicxulub, Mexico.
  • Reference: Fig. 18.31

Consequences of the Asteroid Impact

  • The Yucatán area was enriched with CaSO4 (anhydrite).
  • The asteroid strike launched huge deposits of anhydrite and water.
  • CaSO4+H2O=acidrainCaSO4 + H2O = acid rain
  • Sulfur and other particulates would also hang in the atmosphere, blocking sunlight.

Further Effects of the Asteroid Impact

  • The asteroid impact caused earthquakes and affected volcanic activity, such as the Deccan Traps of India.
  • These would have released gases that changed the climate.
  • Interestingly, these seem to have erupted before the asteroid's impact.

Tsunami and Ecological Disruption

  • The impact would have created a 4 km tall wave.
  • All these features would have tremendously altered Earth.
  • However, not all K-Pg extinctions happened at the same time.
  • The drawn-out process may have had to do with:
    • Disrupted ecological interactions
    • Lack of nutrients
  • Reference: Fig. 18.26

Other Mass Extinctions

  • The Permian-Triassic (P-T) mass extinction is believed to be volcanic.
  • It has been timed to 252 million years ago.
  • It happened simultaneously on land and sea according to the fossil record.
  • The Siberian traps increased atmospheric carbon and warming.
  • O2 levels went down to 13%.
  • Marine O2 and temperature were critically affected too.

Sixth Mass Extinction

  • Are we currently undergoing a sixth mass extinction?
  • How to determine?
  • Describe what sort of data you would collect.
  • It would be impractical to intensely monitor every single species on Earth for the next 30 years.
  • So, you’ll need to be creative.

Humans' Effect on the Planet

  • How to measure the sixth mass extinction?
  • Satellite photography documenting our encroachment on natural lands.
  • Detailed monitoring of species that face extinction threats.
  • Based on these approaches:
    • 100 to 1000 times greater extinction rate than background.
    • Reference: Cowie et al., 2022 Biological Reviews issue with quantifying extinction.

Areas of Greatest Threat

  • Birds are particularly threatened.
  • Reference: Hawkins et al., 2007
  • Vascular plants are highly threatened, especially in certain ecoregions.
  • Reference: Kier et al., 2005
  • Suitability and quality of underlying data.
  • Reference: Kier et al., 2005