exam 1 Flashcards
We can learn about the ocean using data collected by satellites in space.
True
Early Polynesians only traveled within sight of land.
False
traveled as early as 1100 B.C.
1 km = 100 m
Flase
Scientific method
Curiosity, observation and measurement, hypothesis, Experimentation, observation, models, and theory
deepest part of the ocean
Mariana trench located in pacific ocean 6.85 miles Trieste (us navy) 1960 Deep sea challenger
The ocean provides how much of the oxygen we breathe?
70% of oxygen
What is the freezing point of pure water in degrees Celsius?
O
What percent of the Earth is covered by the ocean?
70.8%
subversives and ROVs
Trieste (US navy)
Deep sea challenger
Jason
Alvin
nebular hypothesis
all bodies in our solar system formed from a huge cloud of gas and dust mainly composed of hydrogen
big bang theory
space and time started when
all matter and energy in the universe expanded
from a single point in a cosmic explosion.
• Universe still expanding – measured
with Hubble Space Telescope.
• Approximately 14 billion years old.
Formation of Earths atomsphere
initial atmosphere blown away by solar wind
second atmosphere produced by outgassing
formation of oceans
outgassing
earth cooled water vapor condensed and rained down on Earth
4 billion years ago
early life
3.5 billion years old
hypothesis include
1. Life originated around hydrothermal vents in deep
ocean.
2. Life originated deep below Earth’s surface.
3. Life may have arrived on comets.
Stanley Miller’s experiment
1952 development of life on Earth. Exposed a mixture of gases and water to ultraviolet light and sparks. Organic molecules (amino acids) formed. Showed that vast amounts of organic molecules could have been formed in Earth’s early Oceans.
Heterotrophs
First forms of life.
External food supply.
Energy from breaking down organic molecules in
primordial soup.
Autotrophs
Make their own food
evolved later than heterotrophs
Anaerobic- bacteria (chemosynthesis)
Photosynthetic
autotrophs: Chlorophyll captures
solar energy – led to aerobic (use oxygen)
organisms and extinction of many anaerobic
organisms
Great oxidation Event
2 billion years ago
photosynthetic bacteria releases oxygen to atmosphere
oxidized rocks
ozone builds up
protected earth from UV radiation
Cyanobacteria- earliest aerobic autotrophs
Water: Electrical Polarity
Both hydrogen atoms are on the same side of the oxygen atom.
Slight negative charge on the side of oxygen atoms
slight positive charge on the side of hydrogen atoms
Charge seperation = electrical polarity
arranged according to polarity
dipolar
water
has a positively charged end and a negative end
hydrogen bonds
attraction between hydrogen and oxygen atoms
weaker than covalent bonds with a single water molecule
strong enough to cause cohesion
Cohesion
causes water to stick to itself and have surface tension
water thermal properties
Add or remove energy
To change the state of a substance, the forces
that cause molecules to be attracted to each
other must be broken.
Van der Waals forces
Calorie
amount of heat required to raise the
temperature of 1 g of liquid water by 1 ºC.
Heat
total energy of molecules
Heat may be generated through chemical reactions
such as combustion, from friction or from radioactive
decay.
Temperature
measure of the average
kinetic (moving) energy of the molecules that
make up a substance.
Temperature changes on the addition or removal of
heat energy to a substance.
Solid (ice)
water has rigid structure and does
not flow. Intermolecular bonds are constantly
breaking and reforming as molecules vibrate, but
molecules remain in fixed positions.
Liquid (water)
Water molecules still interact with
one another but have enough kinetic energy to
break bonds and flow.
Gas (water vapor)
molecules have enough
kinetic energy to fully overcome intermolecular
bonds and do not interact except during collisions.
Heat Capacity
amount of heat required to raise
the temperature of 1 gram of any substance 1o C.
Water has a high heat capacity because of hydrogen bonds
rocks and metals have a low heat capacity
Latent heat of melting
energy required to
break intermolecular bonds between ice
molecules to form water; 80 cal g-1
Latent heat of vaporization
energy required
to be added at the boiling point of water to break
the intermolecular bonds and change the state
from a liquid to vapor; 540 cal g-1
identical to the
latent heat of condensation.
Latent heat of condensation
occurs when
water vapor cools sufficiently to condense;
condensation releases energy which can power
thunderstorms and hurricanes.
Latent heat of freezing
Heat released when
liquid water freezes
identical to latent heat of melting
Latent heat of evaporization
conversion of liquid to
gas below its boiling point is called evaporation
Global thermostatic effects
moderate changes in
temperature and drive Earth’s climate, making life possible.
Heat energy is removed from low latitudes and
added to the heat-deficient high latitudes
Mariner- temp. of land moderated by proximity to ocean
Continental- larger fluctuations less influenced by ocean
evaporation condensation cycle
Energy from sun stored in the ocean.
Evaporation removes heat from ocean transferred to
atmosphere.
Water vapor condenses in cooler, higher air to form clouds
and precipitation which
salinity
is the ratio of the mass of dissolved
substances to the mass of the water sample
does not include fine particles in suspension or dissolved organic substances