1ST Flashcards

(37 cards)

1
Q

bigbang theory

A

The top prevailing cosmological model for the early
development of the Universe.

 In the recent past, astronomers have based their new findings
on the beginnings of the universe through cosmic microwave
background (CMB).

 CMB or “afterglow” is a thermal radiation used in
observational cosmology because it is considered the oldest
light in the universe.

 CMB was believed to have been released 380 000 years after
the big bang and is also used to study the composition and
age of the universe.

 When the universe was young, it was denser and hotter (at
around 5.5 billion degrees Celcius)

 It also contained the basic particles of neutrons, electrons,
and protons.

 When the universe got cooler, the basic particles decayed or
combined and created neutral atoms which allowed light to
shine through.

 Clumping of particles, later on, formed the stars and the
galaxies that we have now.

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2
Q

cosmic inflation theory

A

 Proposed by physicists Alan Guth (1974-) and Andrei
Linde (1948-) in the 1980s.

 The theory states that the early universe was a
rapidly expanding bubble of pure vacuum energy.

 After the expansion and cooling due to the inflation,
the potential energy was converted into kinetic
energy of matter and radiation then a big bang
occurred.

 The cosmic inflation theory became an accepted
hypothesis because it answered many puzzles that
arose in the big bang theory which are as follows:

1.) The homogeneity of the objects in space.

2.) The appearance of flatness or smoothness of the
universe.

3.) The formation of stars and star systems in later
years.

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3
Q

steady state theory

A

 First proposed by Sir James Jeans in 1920. It gained
popularity after it was revised by Sir Fred Hoyle, Sir Hermann
Bondi, and Thomas Gold in 1948 as an alternative to the big
bang theory.

 The theory states that the universe is always expanding and
although it is expanding, its appearance does not change.

 It also states that new matter is constantly formed as the
universe continues to expand. The older bodies eventually
became out of sight as a consequence of their increasing
distance and rate of recession.

 This theory further claims that the universe has no beginning
or end in time.

 However, toward the middle of 1960s, evidences that would
contradict the steadiness or the unchanging state of the
universe were brought out.

 One of the evidences was when galactic bodies (quasars &
radio galaxies) were found a long way from the sun at far
distances in space (and found none nearby); it disproved the
idea that similar bodies are created and found everywhere.
Hence, distant objects in space are considered ancient and
the younger universes are found nearer.

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4
Q

creationist theory

A

 This theory states that God, the Supreme Being created the
whole universe out of nothing.

 The proof can be read in the Holy Bible stipulating that God
created the heavens and the Earth including man.

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5
Q

oscilating universe

A

 This theory was proposed by a Russian-born US cosmologist
George Gamow who helped explain the Big Bang theory.

 He said that the expansion of the universe will eventually
come to a halt then it collapses up to the time that the
universe will return to its original form and another Big Bang
will occur. This process will happen as a cycle.

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6
Q

star system

A

It is a small number of stars (most widely recognized as
astronomical objects, and represent the most fundamental
building blocks of galaxies.) that orbit each other bound by
gravitational attraction. It is also called stellar system.

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7
Q

Star Formation

A

Star Formation shapes the appearance of the Universe and provides the
sites for planets.

  1. Initial collapse of an interstellar cloud.
  2. The cloud fragments into clumps . The fragmentation is related to
    turbulence in the collapsing cloud.
  3. The clumps collapse into a stars.
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8
Q

solar system

A

The solar system is a group of objects that interact with
one another, the fundamental interaction for each object
being the one it has with the Sun.

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9
Q

nebular hypothesis

A

 The hypothesis was developed by Immanuel Kant (1724-1804)
and Pierre-Simon Laplace (1749-1827) in the 18th century.

 The most accepted theory among the three.

 It presupposes that around 4.5 billion years ago, a star system
was formed from rotating cloud of gas – or nebula – of
extremely hot gas.

 When the gas cooled, the nebula began to shrink and became

smaller. It rotated fast and cast off rings of gas forming disk-
like shape.

 As the nebula continued to shrink, the rings condensed into
various densities of planets and their satellites.

 The remaining part of the nebula, which has the most mass,
formed the sun.

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10
Q

planetisimal theory

A

 Proposed by Viktor S. Safronov (1917-1999) in 1941 and
developed by T. C. Chamberlin (1843-1928) and F. R. Moulton
(1872-1952).

 The theory states that in the early period of the solar system,
planets were formed from the accretion of small space bodies.

 The gravity of the space bodies attracted space objects until
the effect of their gravity was reduced due to the accretion
which also increased the size of the planetesimals.

 The theory describes the formation of the planets as asserted
in the nebular hypothesis.

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11
Q

tidal theory

A

 Developed by James Jeans (1877-1946) and Sir Harold Jeffreys
(1891-1989).

 According to the theory, a star passed close to the sun where
the tidal force or the secondary effect of gravitational pull
between the passing star and the sun drew large amount of
matter.

 Some of the drawn out matter quickly cooled to become solid
bodies called planetesimals.

 Others grew in size because of colliding and sticking together
with passing objects in space, eventually forming larger
clumps and gathering more and more matter.

 This theory is also backed up by old
meteorites found on earth, chemically
dated back to about 4.5 billion years, the
time approximated to be the formation of
the solar system.
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12
Q

sun

A

•The Sun is a star at the center of our solar
system.
•It is estimated to be 4.5 billion years old.
•It supports all life on Earth through
photosynthesis and is the ultimate source of
all food and fossil fuel.
•It is 333,400 times more massive than the
Earth (this means that 333,400 Earths can
make up the Sun).
•99.86% of all the mass of the solar system is
found in the Sun.
•The core of the Sun is 16 million °C.
•The surface of the Sun is 7000° C

•It takes several hundred thousand years for photons to escape from the dense core and
reach the surface.

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13
Q

Nuclear Fusion in the Sun

A

The Sun is basically a huge ball of hydrogen gas held together by
the gravity created by its own mass. Under the intense pressure
created at the center of the Sun by gravity, hydrogen atoms are
fused together to produce helium. Very simply stated, four hydrogen
atom are fused into one helium, however one helium atom has less
mass than four hydrogen atoms. The fusion process releases enough
energy to account for the lost mass.
The energy released by nuclear fusion in the Sun’s core heats the
Sun. The hot Sun radiates light into space, warming the Earth and
the other planets.

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14
Q

mercury

A

Relative position: 1st planet out from the
sun.

Appearance: Resembles Earth's Moon,
scarred by thousands of impact craters.
There are areas of smooth terrain as
well as cliffs, some soaring a mile
high, formed by ancient impacts.

General composition: Rocky material. It
is a terrestrial planet.

Atmosphere: Almost no atmosphere. The
very little atmosphere that exists is
composed chiefly of oxygen, sodium,
and helium.
Mercury

Size: .054 the volume of the Earth

Planetary satellites (Moons): None

Rotation: 58.65 days (very slow rotation)

Revolution: 88 days to go around the Sun once.

Temperatures: High: 467 °C on the sunny side of the planet. Low: -183 °C on the dark side of the planet.

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15
Q

venus

A

Relative position: 2nd planet out from the sun.

Appearance: It is covered by thick, rapidly
spinning clouds. Due to its thick cloud layer
reflecting sunlight, it is the brightest planet in
the sky

General composition: Rocky material. It
contains an iron core and a molten rocky
mantle. The crust is a solid, rocky material. It
is a terrestrial planet.

Atmosphere: Consists mainly of carbon dioxide,
nitrogen, and droplets of sulfuric acid; it
contains almost no water vapor. This thick
atmosphere traps immense amounts of heat in a
large-scale greenhouse effect.

Size: .88 the volume of the Earth

Planetary satellites (Moons): None

Rotation: -243 days (retrograde)

Revolution: 225 Earth days. Its day is longer than
its year.

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16
Q

earth

A

Relative position: 3rd planet out from the
sun.

Appearance: The Earth looks blue and green
from space with clouds moving through the
atmosphere. The surface of the Earth is
70% water and 30% land.

General composition: Rocky material. It is a
terrestrial planet. It has a nickel-iron core
with a molten mantle and solid rocky crust.

Atmosphere: Mostly oxygen (21%) and
nitrogen (78%). Some argon, carbon
dioxide, and water vapor.

Size: 40,000km (24,8000miles) around at the
equator.

Planetary satellites (Moons): 1 - The Moon

Rotation: 23 hours, 56miutes (1 day)

Revolution: 365.25 days
Earth

Special feature: Earth sustains life as
we know it. Water exists in all three
states (solid, liquid , and gas) on the
Earth. There is a delicate balance
between its oceans, air, land, and life.
17
Q

the moon

A
  • The Moon is the Earth’s only natural satellite.
  • The Moon contains no water and has no atmosphere

• Its has about 1/6 the mass of the Earth, therefore it has
1/6 the gravitational pull of the Earth.

• It is 384 401 km from the Earth.

• It takes 27.32 days to orbit the Earth once.

• The gravitational pull of the Moon is responsible for
the Earth’s tides.

• The surface of the Moon is covered with craters and
flatlands. The craters are due to repeated meteorite
bombardments while the dark, flatlands are the result
of ancient lava flows.

18
Q

mars

A

Relative position: 4th planet out from the sun.
Appearance: Mars appears red due to the iron oxide
in its soil. It has polar ice caps that grow and
recede with the seasons, and it has dust storms,

which cause giant dunes, wind streaks, and wind-
carved features.

General composition: Rocky material. It is a
terrestrial planet.
Atmosphere: Mostly carbon dioxide, nitrogen, and
argon.
Size: .149 times the volume of the Earth.
Planetary satellites (Moons): 2 Moons
Rotation: 24 hours, 33 minutes.
Revolution: 686.67 days.

Special Features: Mars has the largest volcanic mountain in the solar system, Olympus Mons
(27 km high and 600 km across); that are so huge they deform the planet’s roundness;

19
Q

moons of mars

A

Phobos

Gouged by a giant impact crater and
beaten by thousands of meteorite
impacts, Phobos is on a collision
course with Mars. It may collide
with Mars in 50 million years or
break up into a ring.

Deimos

It is also heavily cratered with a
small lumpy appearance.

20
Q

jupiter

A

Relative position: 5th planet out from the sun.

Appearance: It is sometimes called a “mini-solar system”
because of its numerous moons and several rings.
Jupiter appears striped because light and dark belts are
created by strong east-west winds.

General composition: It is a gas giant, meaning it is
mostly made of gases. Jupiter’s core is probably not
solid but a dense, hot liquid with a consistency like thick
soup.

Atmosphere: Mostly hydrogen, helium and methane.

Size: 1316 times the volume of the Earth. It is the planet
with the highest gravity in the solar system.

Planetary satellites (Moons): 63 Moons; some of them
have been named and some have alphanumeric
designations.

Rotation: 9 hours, 54 minutes

Revolution: 11.86 Earth years
Jupiter

Special Feature: The Great Red Spot has existed for at least
100 years, and perhaps longer. It is a hurricane-like storm
on Jupiter. (Galileo reported seeing a similar feature
nearly 400 years ago). Three Earths could fit across the
Great Red Spot.

Moons of Jupiter

  1. Io
  2. Europa
  3. Ganymede
  4. Callisto
  5. Amalthea
  6. Himalia
  7. Elara
  8. Pasiphae
  9. Sinope
  10. Lysithea
  11. Carme
  12. Ananke
  13. Leda
  14. Thebe
  15. Adrastea
  16. Metis
  17. Callirrhoe
  18. Themisto
  19. Megaclite
  20. Taygete
  21. Chaldene
  22. Harpalyke
  23. Kalyke
  24. Iocaste
  25. Erinome
  26. Isonoe
  27. Praxidike
  28. Autonoe
  29. Thyone
  30. Hermippe
  31. Aitne
  32. Eurydome
  33. Euanthe
  34. Euporie
  35. Orthosie
  36. Sponde
  37. Kale
  38. Pasithee
  39. Hegemone
  40. Mneme
  41. Aoede
  42. Thelxinoe
  43. Arche
  44. Kallichore
  45. Helike
  46. Carpo
  47. Eukelade
  48. Cyllene
  49. Kore
  50. S/2003 J2
  51. S/2003 J3
  52. S/2003 J4
  53. S/2000 J11
  54. S/2000 J5
  55. S/2003 J9
  56. S/2003 J10
  57. S/2003 J12
  58. S/2003 J15
  59. S/2003 J16
  60. S/2003 J17
  61. S/2003 J18
  62. S/2003 J19
  63. S/2003 J23
21
Q

saturn

A

Relative position: 6th planet out from the sun.
Appearance: Saturn has a large system of
rings, and the yellow and gold bands in its
atmosphere are caused by super-fast winds
combined with heat rising from its interior.
General composition: It is a Gas giant,
meaning it is mostly made of the gases
hydrogen and helium.
Density: .70 gm/cm3

(This low density means
that Saturn could float on water if there was
a body of water big enough).
Atmosphere: Mostly hydrogen and helium.
Size: 755 times the volume of the Earth.
Planetary satellites (Moons): 60 Moons; some
have been named and others have
alphanumeric designations
Rotation: 10 hours, 38 minutes
Revolution: 29.45 Earth years

Special feature: Saturn’s ring system is the most
extensive and complex in our solar system; it extends
hundreds of thousands of kilometers from the planet.
The rings are mostly water ice with particles ranging in
size from a few micrometers to several tens of meters.

Moons of Saturn

  1. Mimas
  2. Enceladus
  3. Tethys
  4. Dione
  5. Rhea
  6. Titan- Saturn’s
    largest moon
  7. Hyperion
  8. Iapetus
  9. Erriapus
  10. Phoebe
  11. Janus
  12. Epimetheus
  13. Helene
  14. Telesto
  15. Calypso
  16. Kiviuq
  17. Atlas
  18. Prometheus
  19. Pandora
  20. Pan
  21. Ymir
  22. Paaliaq
  23. Tarvos
  24. Ijiraq
  25. Suttungr
  26. Mundilfari
  27. Albiorix
  28. Skathi
  29. Siarnaq
  30. Thrymr
  31. Narvi
  32. Methone
  33. Pallene
  34. Polydeuces
  35. Daphnis
  36. Aegir
  37. Bebhionn
  38. Bergelmir
  39. Bestla
  40. Farbauti
  41. Fenrir
  42. Fornjot
  43. Hati
  44. Hyrokkin
  45. Kari
  46. Loge
  47. Skoll
  48. Surtur
  49. S/2004 S7
  50. S/2004 S12
  51. S/2004 S13
  52. S/2004 S17
  53. S/2006 S1
  54. S/2006 S3
  55. Greip
  56. Jarnsaxa
  57. Tarqeq
  58. S/2007 S2
  59. S/2007 S3
  60. Anthe
22
Q

uranus

A

Relative position: 7th planet out from the sun.
Appearance: It has a blue-green color from the methane
gas above the deeper clouds. Methane absorbs red
light and reflects blue light. It does have a small
system of rings.
General composition: It is a Gas giant, meaning it is
mostly made of the gases hydrogen and helium, with
a small amount of methane and traces of water and
ammonia. It has no solid surface, but it does contain
a liquid core made mostly of “icy” materials (water,
methane, and ammonia)
Atmosphere: Mostly hydrogen, helium, and methane.
Size: 52 times the volume of the Earth.
Planetary satellites (Moons): 27 Moons
Rotation: 17 hours, 11 minutes
Revolution: 84.02 Earth years

Uranus

Special feature: Uranus’ axis is tilted so that it seems to
rotate on its side. This tilt gives it seasons that last over
twenty years.

Moons of Uranus

  1. Cordelia
  2. Ophelia
  3. Bianca
  4. Cressida
  5. Desdemona
  6. Juliet
  7. Portia
  8. Rosalind
  9. Mab
  10. Belinda
  11. Perdita
  12. Puck
  13. Cupid
  14. Miranda
  15. Francisco
  16. Ariel
  17. Umbriel
  18. Titania
  19. Oberon
  20. Caliban
  21. Stephano
  22. Trinculo
  23. Sycorax
  24. Margaret
  25. Prospero
  26. Setebos
  27. Ferdinand
23
Q

neptune

A

Relative position: 8th planet out from the sun.

Appearance: Neptune has a blue color because of the
methane in its atmosphere. The methane reflects
blue light while it absorbs red light. It has a small
system of rings and periodically Great Dark Spots
(hurricane-like storms) appear.

General composition: It is a Gas giant, meaning it is
mostly made of the gases hydrogen, helium, and
methane. It has no solid surface, but its liquid core
is composed of water and other “melted ices.”

Atmosphere: Mostly hydrogen, helium,and methane.

Size: 44 times the volume of the Earth.

Planetary satellites (Moons): 13 Moons

Rotation: 16 hours, 4 minutes

Special features: Neptune is actually the Revolution: 164.79 Earth years
farthest planet from the Sun for a 20-year
period.

Moons of Neptune

  1. Triton
  2. Nereid
  3. Naiad
  4. Thalassa
  5. Despina
  6. Galatea
  7. Larissa
  8. Proteus
  9. Halimede
  10. Psamathe
  11. Sao
  12. Laomedeia
  13. Neso
24
Q

pluto

A

Relative position: 9th planet out from the sun.
Appearance: A large frozen ball of ice.
General composition: Rocky core surrounded by
water ice.
Density: 2.0 gm/cm3
Atmosphere: Frozen most of the time. When it
is closest to the Sun the bright layer of frozen
methane, nitrogen, and carbon monoxide
thaws out and gives it a thin atmosphere.
Size: .005 the volume of the Earth. It is the
planet with the lowest gravity in the solar
system.
Planetary satellites (Moons): 3

  1. Charon
  2. Hydra
  3. Nix

Rotation: -6.39 days
Revolution: 247.9 Earth years

25
asteroids
• Asteroids are either rocky or metallic objects that orbit the Sun. They are too small to considered planets but are sometimes called planetoids. • They can be anywhere from the size of a pebble up to a 1000km (620 miles) in diameter; the asteroid Ceres is an example of an asteroid that is this large. • They have been found inside Earth’s orbit and all the way out past Saturn’s orbit. Most asteroids, however, are located in the asteroid belt which exists between the orbit’s of Mars and Jupiter.
26
comets
 Comets - small, fragile, irregular - shaped body composed of a mixture of non -volatile grains and frozen gases. ```  Their orbits are elliptical (oval) or parabolic (U -shaped). The orbit brings them in very close to the Sun and swings them far out into space, sometimes out past Pluto. ```  As comets approach the Sun, radiation from the Sun evaporates the ice and gases, creating the lone tail. The closer to the Sun, the longer the tail of the comet. The tail of the comet always faces away from the Sun because of the solar wind coming from the Sun.
27
Meteors, Meteoroids, and Meteorites
• Meteoroids - asteroids that are on a collision course with Earth. • Meteor - streak of light created when a meteoroid strikes our atmosphere at high velocity and friction causes the chunk of space matter to burn up. • Meteorite - what is left that strikes the Earth’s surface if the meteoroid does not burn up completely. • 92.8% of all meteorites are composed of silicate (stone), and 5.7% are composed of iron and nickel; the rest are a mixture of the three materials. • Stony meteorites are the hardest to identify since they look very much like terrestrial rocks.
28
earth system
is essentially a closed system. It receives energy from the sun and returns some of this energy to space.
29
geosphere
 The portion of Earth that includes the interior structure, rocks and minerals, landforms, and all physical processes on land that shape the Earth’s surface.  All the continents and ocean floor are also considered parts of the geosphere.  Scientists that study this part of earth are called geologists.
30
earth's internal structure
 The Crust is like the skin of an apple. It is very thin in comparison to the other layers of Earth.  The crust is only about 3-5 miles (8 kilometers) thick under the oceans(oceanic crust) and about 25 miles (32 kilometers) thick under the continents (continental crust).  Most of the crust is composed of eight elements namely: 1. Oxygen 5. Calcium 2. Silicon 6. Sodium 3. Aluminum 7. Potassium 4. Iron 8. Magnesium  The mantle is the solid rock and is the largest part of Earth.  Earth's mantle is a silicate rocky shell with an average thickness of 2,886 kilometers (1,793 mi).  It lies between the extremely hot core and the thin outer layer of the crust.  The mantle makes up about 84% of Earth's volume.  It is predominantly solid but in geological time it behaves as a very viscous fluid.  The outer core of the Earth is a liquid layer about 2,266 kilometers thick.  It is made of iron (Fe) and nickel (Ni).  The inner core is the Earth's innermost part and according to seismological studies, it has been believed to be primarily a solid ball with a radius of about 1220 kilometers, or 768 miles (about 70% of the Moon's radius).  It is composed of an iron–nickel alloy and some light elements.
31
discontinuity
``` • Just above the upper mantle and still part of the crust is the Mohorovicic discontinuity or simply Moho. • It was termed as discontinuity because the seismic waves behaved differently as they traveled through this layer. • Moho is now recognized as the transitional boundary that divides the crust and the mantle. ``` ``` Andrija Mohorovicic (1857-1936) -was an Croatian meteorologist and seismologist who suggested that there are lies a boundary between the crust and boundary and was later named as the Mohorovicic discontinuity or the Moho. ``` ``` • The Gutenberg discontinuity serves as a transitional boundary between the lower mantle and the outer core. • This boundary does not remain constant because of changes in heat flow. • When heat in mantle dissipates, the molten core gradually solidifies and shrinks, moving this boundary deeper and deeper within Earth’s core. ``` ``` Beno Gutenberg (1889-1960) -was a German seismologist who discovered the Gutenberg boundary. ``` • The Lehmann discontinuity is a transitional boundary between the inner and outer core. ``` Inge Lehmann (1888-1993) -was a Danish seismologist who in 1936, asserted that Earth’s core is not just a single molten sphere but it comes with a solid inner core based on seismic data. ```
32
atmosphere
 The atmosphere is the thin gaseous layer that envelopes the lithosphere.  The present atmosphere is composed of 78% nitrogen (N), 21% oxygen (O2), 0.9% argon, and trace amount of other gases.  One of the most important processes by which the heat on the Earth's surface is redistributed is through atmospheric circulation.  There is also a constant exchange of heat and moisture between the atmosphere and the hydrosphere through the hydrologic cycle.
33
The Four Layers of the Atmosphere
 Troposphere ```  this layer is considered to be the densest among the other layers. Because temperatures drops with altitude, warm air on the surface of Earth rises readily.  Air molecules travel up and back down causing the formation of clouds and eventually rain from the moisture in the air.  Almost all weather variations occur within the troposphere.  prior to reaching the next layer above the troposphere is a thin buffer zone called the tropopause. ``` Stratosphere ```  the air in this layer has strong , steady horizontal winds which is advantageous to long distance flights.  At its upper region is the ozone layer at about 6.2 miles or about 33 000 feet above Earth’s surface which contain a high concentration of ozone.  another thin buffer zone exists before the next layer above the stratosphere and this zone is called the stratopause. ``` ```  Mesosphere  this is the layer above the stratosphere. The temperature here reaches a minimum of -90 °C and is considered to be the coldest layer.  This layer is important in protecting the Earth from planetary debris.  the thin buffer zone above the mesosphere is called the mesopause. This zone is actually the coldest region in the atmosphere. ``` Thermosphere  this layer is the hottest layer because of its absorption of highly energetic solar heat.  the lower part of the thermosphere is the ionosphere where most collision of oxygen and nitrogen particles are electrically charged by the solar wind.  Solar wind is a stream of energized, charged particles flowing from the sun.  Charged particles- are called ions, consists of protons and electrons with high kinetic energy and the high temperature of the corona.  there exists a thermopause above the thermosphere that also serves as a buffer zone which separates the
34
hydrosphere
 About 70% of the Earth is covered with liquid water (hydrosphere) and much of it is in the form of ocean water.  Only 3% of Earth's water is fresh: two-thirds are in the form of ice, and the remaining one-third is present in streams, lakes, and groundwater.
35
characteristic of water
1. Water could be in liquid form, not just solid and gas. 2. Water has a neutral pH. 3. Water is a good conductor of heat and energy. 4. Water has a specific heat. 5. Water is a universal solvent.
36
Distribution of Waters on Earth
 Surface water may be either marine water or fresh water. Marine water has higher salt content and is found in larger bodies of water such as oceans, seas, bays. Freshwater are those in lakes, rivers, springs and falls. Has a salt lower content. It is the best source of drinking water for all organisms.  Ground water is the water found beneath Earth’s surface where there are spaces in the soil or fractures in rocks.
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Scientists with Significant Contribution to Our Knowledge of Earth
James Hutton (1726-1797) -is recognized as the founder of modern geology. He was a Scottish naturalist and farmer. Charles Darwin (1809-1882) -was an English naturalist known for the theory of evolution. Alexander Oparin (1894-1980) -was a Soviet biochemist who proposed the primordial soup theory in 1924 to explain the origin of life on Earth . ``` Stanley Miller (1930-2007) -was a Jewish- American chemist who conducted an experiment in 1952 to test the hypothesis of Oparin’s primordial theory.. ```