100 Earth Facts: The Big List of Facts About Earth
Earth needs no introduction.
From its origin, to its inevitable future, the story of Earth is greatest story ever told.
So if you’re looking to boost your knowledge of our planet….
You’ll really enjoy this list of 100 Earth facts.
Let’s get started.
1 The Big Bang created all matter in the universe
The physics we use does not apply to the creation of the universe. From the initial phases of the Big Bang, the universe now holds a mammoth collection of galaxies, stars, planets and other solar remnant.
We know this because we observe them using the Kepler and Hubble Telescopes. On the grand scale of things, Earth is tiny in comparison.
2 The universe is expanding into the unknown
We know the universe is still expanding because we measure the redshift of light. Redshift means that light stretches when objects move away from you.
Alternatively, it’s blue shift when moving toward. It’s like the Doppler Effect which uses sound waves, but redshift uses light.
3 Welcome to the Milky Way Galaxy
Galaxies are flat because things that rotate flatten out on the rotational access. For example, Earth is longer at the equator axis because of its rotation.
Galaxies are also rotating around some point in space. This is likely where the Big Bang occurred.
4 Gravity sculpts solar systems
Gravity is the constructor of our planet 4.6 billion years ago. Depending where you are on Earth, gravity varies.
For example, gravity is 9.764 m/s2 in Peru and 9.834 m/s2 in the Arctic. This is because mass (like mountains) and the bulge at the equator amplifies it.
5 Constructing a planet
But the sun couldn’t pull in heavier elements because of their mass. They spiraled and gelled together into planets of their own. Earth coalesced to form spheres of their own. The heaviest material like iron and zinc sank to the core.
Finally, lighter material remained on top to form a crust. The two opposing forces of Jupiter and the sun counteracted each other stabilizing the terrestrial planets and an asteroid belt between.
6 Third rock from the sun
It takes light 8 minutes and 20 seconds (1 astronomical unit) to reach us. Earth is the only planet known to harbor life because of the healthy portion of UV rays that heats it.
Earth has had 2 major phases. A brief period of heating up from the “heavy bombardment stage”. And everything since which cooled the Earth. The early stage was fast and catastrophic with tons of impacts and tremendous heating.
7 Earth is a red marble
Earth spun with incredibly high velocity, nearly 3 times as fast as it did today. Like a scene from a Michael Bay movie, meteors and asteroids pelted Earth for millions of years.
This violent era was the late heavy bombardment stage – a sight unseen from the human eye. From red to the blue marble, it was a dawn of a new age because of the formation of the moon.
8 Clues to our origin
This is why gaze toward the moon. Because plate tectonics don’t exist on the moon, the impacts from this violent period are still visible as craters. There are other clues about the formation of our solar system.
For example, we probe orbiting comets to study the origin of water. Finally, we explore Mars to delve into the necessary conditions for life to exist in the universe.
9 Earth’s interior has layers
The core (2,890-6,360 km) of Earth is like the pit of a cherry because it’s solid. The mantle (35-2,890 km) is like the cherry which is mostly solid and behaves like a viscous fluid.
Finally, the crust (0-35 km) is the outermost shell. It’s rigid because lighter material remained at the surface. But the heavier material like iron and zinc sank to the core.
10 We use earthquakes to peak into Earth’s core
Depending on the type of rock, waves either speed up or slow down. If the rock is cold, waves travel quickly. But if rocks are hot, waves travel slowly.
From seismic stations around the world, we listen to the ground shaking like a tape recorder. From these tomography readings, we produce 3D models of the Earth’s interior.
11 Earth meet moon
After the moon collided with Earth, it tilted it on its axis giving seasons. In tandem, they control tides, slow rotational speed and stabilize Earth from wobbling.
There’s just one moon that orbits Earth. But if you stepped foot on Jupiter, you would see 63!
12 The 4 seasons
This collision promptly delivered seasons to Earth. If it wasn’t for the moon, Earth’s climate would be unpredictable and have wild shifts.
This is because the gravitational pull of the moon has a stabilizing effect for Earth preventing it from wobbling like a top.
13 Earth’s poles North and South
If you were to travel to the North Pole, it’s nearly impossible to install a physical marker there. This is because the North Pole is covered by moving ice in the Arctic Ocean.
But the South Pole is currently positioned on the continental landmass of Antarctica. Even though Antarctica moves only a few meters a year, we have marked the true South with a permanent marker station.
14 Earth is the densest planet
Finally, nickel (2%), sulfur (2%), calcium (1%) and aluminum (1%) make up most of the rest. In terms of mass, gas giants like Jupiter dwarfs Earth.
The colossal heavyweight Jupiter radius is nearly 70,000 km compared to Earth’s measly 6,371 km.
15 Our magnetic field
Inside Earth, the solid core heats the outer liquid layer. As a result, this produces a geodynamo and convection currents which is our magnetic field.
Without a magnetic field, our skin would be unguarded from harmful radiation. Also, solar flares from the sun would constantly cut off our communication systems.
16 A healthy dose of solar radiation
When incoming energy from the sun is absorbed by the Earth system, Earth warms. When the sun’s energy is reflected back into space, Earth avoids warming.
When absorbed energy is released back into space, Earth cools. Natural and human causes can influence Earth’s energy balance.
17 Earth is in the Goldilocks zone
In other words, because Earth receives a hearty portion of sun’s rays (1 astronomical unit), it can sustain life. Even here in our Milky Way galaxy, at least 10 possible habitable planets are within the Goldilocks zone.
This means that only light years away, there is a glimmer of hope that other life exists.
18 Nitrogen outnumbers oxygen 3 to 1
Why so much nitrogen? Simply, it’s just because it’s what was here when the Earth formed. But only is there a sizable amount of nitrogen in the atmosphere, but it’s entangled in our soil fertilizing plants.
Earth’s atmosphere composition largely consists of nitrogen, oxygen, argon, carbon dioxide and water vapor.
19 Our changing atmosphere
But after oxygen filled the air, it created a habitable planet. Since early Earth, oxygen levels have changed significantly.
For example, free oxygen levels peaked just before the age dinosaurs. Now, Earth’s blue skies are picturesque. We have oxygen to thank for its impeccable beauty.
20 Our first oceans
Because Earth’s interior contains minerals with hydrogen and oxygen, volcanoes continual “degassed” releasing H2O as water vapor. If it weren’t for the process of degassing our planet through volcanoes, we wouldn’t have any air to breathe.
Volcanoes erupts and lava spews out, but it also ejects gas into the atmosphere.
21 One full rotation takes 24 hours
That makes Earth’s rotation faster than a bullet train but not a speeding bullet. But our bodies are so used if to it that we don’t feel its speed. Earth’s rotation is a pace-setter for our sleep patterns.
If you shine a flashlight on a spinning top, the side lit up is daytime. The dark side is night-time. That’s how our day-night cycles work with the sun as our flashlight.
22 Earth is not a perfect sphere
As the Earth spins on its axis, it flattens at the poles and widens at the equator. Sir Isaac Newton proposed the centrifugal force causes the planet to bulge at the equator and somewhat squash at the poles.
This is why geographers model the Earth as an ellipsoid, which is a sphere slightly flattened at the poles.
23 Ocean tides and the moon
When the Earth rotates, the bulge shifts on both sides of the planet according to the position of the moon. In full swing, this causes sea levels to rise and fall which are ocean tides.
The sun has lesser effect than the moon. Even though the moon is smaller, the moon is closer. So this means that it’s pull is stronger than the sun.
24 Radioactive isotopes put Earth on a light simmer
These four isotopes are uranium-238 (238U), uranium-235 (235U), thorium-232 (232Th), and potassium-40 (40K). Each number in these radioactive isotopes corresponds to the number of protons and neutrons in its nucleus.
Because of these 4 isotopes, Earth is geologically active and maintains a cozy temperature. The majority of heat transfer is from mid-oceanic ridges and the least is continental interiors.
25 Heat transfer from convection cycles
Eventually, this movement of hot to cold creates a circular motion which is the convection cycle.
Beneath the crust, the convection cycle occurs in the mantle. Because the plastic-like “asthenosphere” acts as a liquid, it makes the convection cycle possible.
26 The lithosphere rides on the asthenosphere
Soon after dramatic period of Earth heating, the Earth started to cool down. This was when the solid lithosphere layer began to form as continents began to rise up out of the mantle.
The asthenosphere is the untold story about how its fluidity facilitates plate tectonics.
27 Plate tectonics create new rock
Like a giant conveyor belt, one end of a plate is sinking into the Earth transporting whatever is on top of it. At the opposite end, new rock rises from the mantle.
Plate tectonics are the mechanism that recycles Earth’s lithosphere. This breakthrough discovery transformed geology as we know it.
28 Building mountains and orogenies
This geologic process of vertical upheaving is the orogenies or mountain building events. Since the beginning of Earth, plate tectonics have carved out chains of mountains which have reshaped the landscape inside and out.
While young rock appear and disappear, cratons are stable pieces of continent that have lasted over 1 billion years old.
29 Tearing down mountains
By mostly water, wind and ice, mass wasting is the removal of rock due to erosion. Then, it involves the transport of sediments downhill due to gravity.
Currently, Mount Everest is thrusting upwards faster than it being eroded away. But in hundreds of millions of years time, erosion could take its toll shortening it by millimeters each year.
30 A breath of fresh air
Long ago, tiny, microscopic cyanobacteria flourished in ocean environments. They evolved to carry out photosynthesis anaerobically. The key to their existence was that they didn’t need oxygen to survive.
As a by-product, cyanobacteria released oxygen which was toxic for them. As oxygen filled the oceans then the atmosphere, this event was the great oxygenation event. This paved the way for aerobic organisms to carry the torch.
31 A struggle for constant oxygen
Because iron rusts when it reacts with oxygen, these layers were red. So the red (oxidized) layers mark a time when there was oxygen. The alternating layers in Banded Iron Formations (BIF) consist of red minerals (oxidized) and (unoxidized) black iron.
These remarkable formations give a sneak peak of how oxygenation was just starting to get a foothold in this geologic period.
32 An ozone layer like sunscreen
Ozone ranges from 6 to 10 kilometers in the stratosphere. Cross the line, and suddenly there’s less as you go upwards. Ozone is good up high, bad down low.
This colorless gas is made up of three oxygen atoms. It’s the first line of defense that arms us against ultraviolet rays. If you strip Earth of its ozone, you strip it from most life forms.
33 A nearly closed system
We lose some hydrogen from the atmosphere due to its escape velocity. And we get the occasional meteor strike.
But in general, Earth is a closed system because it doesn’t exchange matter from or to the outside. Earth exchanges energy due to incoming solar radiation but little matter leaves or enters.
34 The rock cycle recycles the crust
Like a well-oiled machine, rocks transform from igneous, sedimentary to metamorphic over long periods of time.
This process where rocks are created, altered and formed again is the rock cycle.
35 Volcanoes form igneous rocks
Once you pull the cork, the volcano erupts from the mouth spewing lava. Like wax dripping down the side of a candle, igneous rocks form.
So hot lava drips on the side of volcanoes then cools, hardens and become igneous rocks like granite and feldspar. Without igneous rocks, there wouldn’t be the rock cycle.
36 Metamorphic rocks from pressure
When it’s metamorphosed, it’s soft and pliable like cookie dough. This intense pressure for metamorphic rocks comes from inside Earth.
Earth’s major mountain chains contain metamorphic rocks because it’s at plate tectonics boundaries where this intense pressure exists.
37 Sedimentary rocks from compacted sediments
This happens because shorelines move back and forth compacting material below like a steam roller. The new layers of sedimentary rock are on top and the older layers on the bottom.
Like glue, each successive layer cements over tens of millions of years. For example, the Grand Canyon has stacks upon stacks of sedimentary rocks dating back to 2 billion years ago.
38 Youngest rock is oceanic crust
When the lava hardens, it becomes dark igneous rock “basalt” at rift volcanoes. Because divergent plates fills in the gaps with basalt, oceanic crust is young geologically.
Over time, the plates grow at oceanic crust and older rock is pushed away from mid-oceanic ridges.
39 Earth’s most prominent feature is hidden beneath the ocean
These occur at divergent plates where plates move away from each other. On the flip side, trenches form where plates move toward each other.
For example, the Mariana trench is the deepest natural point in the world. This is due to the subduction that occurs at two convergent plates.
40 LUCA is the one common descendant
Around 4 billion years ago, two unicellular groups existed as bacteria and archaea. Scientists have found that certain protein families likely descended from the organism.
LUCA found withstand hot temperatures. This means they likely thrived in an iron-sulfur rich lifestyle like deep-sea hydrothermal vents.
41 Your identity is in the genes
The truth is: we don’t know the origin of DNA. And we don’t even know if RNA came before. In primordial soup, this is where organic compounds and amino acids had the right conditions to synthesize from inorganic matter.
In hydrothermal vents beneath the ocean floor, this is where it’s believed to have the necessary building blocks for life.
42 Complex life from endosymbiosis
In turn, the mitochondrion leverages the nutrient-rich surrounding of the prokaryote. And in return, the prokaryote energizes from the mitochondria during its residence. As both symbiotically gain from the encounter, they asexually multiply and evolve in this configuration.
In conclusion, mitochondria once lived free but are now part of complex cells through endosymbiosis.
43 Cambrian explosion and life diversification
This was the first time in geologic history that we could identify life from fossilized animals. Everything else before this era was Precambrian without hard body parts.
The Cambrian explosion was the roots of life that sparked a colossal amount of diversity in oceans and land.
44 Fossil records are like frozen photographs
Every fossil was living before our time untouched for centuries. Like frozen photographs in the past, we piece together the geologic past with fossils.
Every fossil is like a puzzle piece that we link to the evolution of life. By examining a simple imprint in rock, we understand ancient supercontinents and continental drift.
45 Fossils don’t exist in 88% of Earth’s history
This marked a time that a wide array of life forms evolved. For example, we’ve uncovered fossils with shells or exoskeletons during this era.
This means that if you look at Earth’s geological timeline, complex life did not exist for more than 88% of it.
46 Water covers 70% of the planet
While 3% is freshwater, 97% is salted. Of the 3% freshwater, most is locked in glaciers or groundwater.
Water is essential for us because it drives the hydrologic cycle, weather patterns and all life on Earth.
47 Water changes states from gas, liquid and water
We have so much water on the surface that it’s incorporated in the water cycle, weather and biology. From a liquid state, water evaporates into a gas or freezes into ice.
Like water dripping down a chilled glass of water, condensation goes from a gas to liquid state. Finally, melting is when the sun beams down on ice converting it to a liquid.
48 Water is on the move in the hydrological cycle
And it’s all driven by the sun’s energy. The main focus is how water is stored – in the atmosphere, glaciers, oceans, plants and humans.
Most evaporation takes place at oceans. It’s the coriolis effect that moves it.
49 The Coriolis Effect drives air circulation
This phenomenon is “wind”. If Earth didn’t rotate, warm air at the equator would simply transfer to the poles. But because the Earth rotates, air starts to swirl like a merry-go-round.
This is the Coriolis Effect that causes storms to veer counter-clockwise in the northern hemisphere and clockwise in the southern hemisphere.
50 A weather-driven atmosphere
Like squeezing a sponge, it redistributes water in the form of rain, sleet and snow. This has influenced migration patterns and the type of vegetation that grows.
One billion tons of water falls every minute on Earth. Severe weather like tornadoes, hurricanes and flooding have displaced people from homes costing billions in damage.
51 A layered atmosphere
In general, the atmosphere is thickest closer to the surface. If you go upwards 5500 meters, air pressure is half that at sea level. So this means you have to breathe about twice as much to get same amount of oxygen. We live in the troposphere where all weather occurs.
Next, the jet stream and airplanes fly in the stratosphere at 12-50 km altitude. The mesosphere is the coldest layer extending from 50-85 km upwards. Finally, the thermosphere is where UV radiation heats up.
52 Groundwater as a hidden freshwater supply
Groundwater has more than 100 times the amount of freshwater than lakes and streams combined. Groundwater is hard to get out of the ground, slow to recharge and is easily contaminated.
That’s why groundwater is a delicate resource that we use as a rainy-day fund and draw in times of need. Pardon the pun.
53 Ocean currents push water across the globe
From the equator, hot water pushes outward to the south and north pole. At the same time, cold water from the north and south poles collide with this warm water. Because the Earth is rotating, water flows in a circular pattern.
This is why ocean currents move clockwise in the northern hemisphere and counter-clockwise in the southern hemisphere. While wind drives surface ocean currents, temperature and salt gradients mostly influence deep ocean currents.
54 Earth’s background noise
These oscillations are due to ocean waves constantly crashing into continents. Earth’s constant hum is because masses shake back and forth like a metronome.
And during storms, it worsens as the reverberations are amplified.
55 Photosynthesis and food synthesis
Without water or CO2, you choke the plant from the essential building blocks that is the plants structure. So water is H2O which provides oxygen and hydrogen. Carbon dioxide is CO2 which provides carbon and oxygen.
The plants use solar energy to break apart the carbon dioxide in the air, and use the carbon for plant material in turn releasing the oxygen. This cycle is the short-term carbon cycle.
56 The short-term carbon cycle
In turn, this produces O2 back into the air. Carbon fuels all living things. For example, animals consume food for energy using O2 and giving off CO2.
Then, it goes back again through the same process again. So the short-term carbon cycle describes how carbon goes from an inorganic compound like CO2 into an organic compound like C6H12O6.
57 The long-term carbon cycle
Instead of carbon converting into sugars, carbon is re-purposed into fossil fuels like coal. When plants are buried and compacted over millions of years, they become hydrocarbons.
When you drive your gas-powered car, you tap into Earth’s carbon reserves deposited hundreds of million years ago.
58 Coal reserves from buried plants
As we unlock these reserves, they hold incalculable worth. We harness their power and release into the atmosphere. After usage, it becomes part of the short and long-term carbon cycle again.
From here, it takes millions of years to become a fossil fuel again or just several to take part in the photosynthesis of a plant.
59 The greenhouse effect is essential to life
Now, the bad news. Because we put too much of it in the air, it amplifies the greenhouse effect and less solar radiation is radiating back to space.
Too much of a bad thing can leave everlasting consequences for our planet.
60 Trees grow from top down
Then, it produces sugars to create the trunk and other structures of the tree. The nutrients that plants get from soils mostly aren’t used as part of the main body and structure of a tree.
Plants use these nutrients for the more complex structures within plants, such as functional proteins and enzymes. This means that most of the dry mass of trees is made from the contents of the air.
61 Gas burnt in your car ends up in plant material
So that same weight from the tank of gasoline gets converted into wood or plant material by photosynthesis.
Given how many cars are being driven daily, plants have access to plenty of “material” for their growth. They just need the ideal conditions to grow.
62 Life evolves on Earth
This is because life evolved in some of the toughest conditions like an overabundance of water and nutrient deficient soils. Over time, plants, animals and fungi have developed immunity to harmful bacteria and viruses from these harsh conditions.
This is because whatever doesn’t work just doesn’t survive. Evolution does the work. This is why we find some of the most resistant chemicals for medicine in tropical rainforests.
63 Dinosaurs dominated for 160 million years
Higher oxygen levels meant more size and mass. There is varying opinion on oxygen levels during the age of dinosaurs. Regardless, these reptile-like mammals grew to extraordinary size.
Ultimately, the demise of dinosaurs was a 6-mile wide asteroid known as the Cretaceous–Paleogene extinction event. Temperatures began to plummet because a dust cloud blocked the sun.
64 Mass extinctions are common in nature
For example, ocean/atmosphere chemistry, climate change, volcanic activity and meteor/asteroid impacts had fatal consequences. No matter how far back you look, nature has found its way to reshuffle the deck.
Large mammals are at greater risk. For example, giant sloths, mastodons and saber-toothed tigers became extinct only about 10,000 years ago. They just couldn’t find a way to outmuscle nature.
65 The supercontinent cycle
On average, continents move about 1 inch per year. Plate tectonics drive the reshaping of continents. Inch by inch, this accounts for incredibly long distances over millions of years.
Long ago, cratons merged to create vast stretches of land. For example, Vaalbara, Ur and most recently Pangaea (sometimes spelled Pangea) took part in the supercontinent cycle.
66 Supercontinents and superoceans
From coast to coast, Pangaea was surrounded by the superocean Panthalassa. Gradually, continental drift teared the supercontinent apart into our current placement of continents.
Today, we pick up the pieces and look at the clues of Pangaea. For example, notice the striking similarities of continental boundaries aligning in a world map.
67 Dinosaur fossils from Pangea
We know this because we can find the same fossils on separate continents today. We see fossils of the same land herbivores today on separate continents that couldn’t fly or swim.
The reason is because they lived on Pangaea and over time it separated. To this day, scientists have kept a thorough record documenting each fossil discovery.
68 The geologic time scale
We work in hours, days, months and years. But the Earth works in decades, centuries and millions of years.
Like chapters in a book, geologists partition Earth’s history into periods, eras and epochs. Each block of geologic time has a notable start and end. So that means that timing is everything when it comes to the geologic time scale.
69 Meteorites date the Earth as 4.5B years old
Despite the challenges of grappling with geologic time, we can come up with a decent estimate of Earth’s age by studying meteorites.
Meteorites are remnants when all the planets were forming. Some of them still land on the planet today. By dating meteorites, we find that the oldest rocks are often 4.5 billion or so years old.
70 Carbon dating uncovers age
By examining the ratio between the two for dead matter, we can estimate age with carbon dating. But there are limitations to measuring beta decay.
At a certain age (60,000 years or so in history), there isn’t enough carbon-14 that remains from the organism to make an accurate estimate.
71 The Grand Canyon reveals Earth’s age
Like a stack of pancakes, younger rock layers pile on top of older layers. We use the law of superposition to reveal Earth’s age. For example, the base of the Grand Canyon are Precambrian basement rocks.
These were formed from flowing magma which cooled and hardened about 1.8 billion years ago. Most of the rocks on top are sedimentary like shale, limestone and sandstone.
72 Magnetic pole reversals
On average, it takes 250,000 years for Earth’s magnetic north to flip polarity. As shown in rocks, magnetic pole reversals are one of the key gateways to recognizing the past.
On average, pole reversals occur every 200,000 to 300,000 years. We may be due for one soon.
73 Planetary (Chandler) Wobbles
Precession occurs because the Earth is not a perfect sphere. It flattens out at the poles. But the Chandler Wobble actives a wobble that is minuscule.
It’s just 20 feet in deviation at the North Pole. No longer a mystery, the key driver of wobbling is temperature and salinity changes at the bottom of the ocean.
74 Ice ages are periodic
It’s close to circular now. But like a pendulum, eccentricity will swing back the other way. It’s because Venus is so close and Jupiter is so large that gravity affects its orbit.
There’s been a noticeable trend in climate, temperature and seasons due to the Milankovitch cycle.
75 Earth was a snowball
Ice ages happen for several reasons. In the eyes of Milankovitch, Earth is prone to ice ages because of how its cyclical movements affects climate.
At least, this is reasonable to assume for the last ice age 10,000 years ago. Atmospheric chemistry, solar output and ocean currents can trigger ice ages.
76 Glaciers chisel away the land like a rake
They tore mountains down carrying vast amount of rocks from the continent across the border. Continental glaciers chisel away at the land leaving its fingerprint in the land.
For example, Long Island, New York is the result of glacial debris from the sediment dumping of a glacier terminal moraine.
77 Continents are still rebounding from the last ice age
After the ice melted, Canada began lifting. We know this because we measure its vertical motion with GPS. Imagine squeezing a sponge and watching it return to its shape.
Similarly, isostatic rebound is quick at first, then slows down. This process of glacier rebound is due to the asthenosphere behaving in a fluid manner. Because ice had been removed, the compressional force no longer exists.
78 Humans have only explored 20% of oceans
So that means we have oceans mapped at about 100 meters resolution which is the same as our surface maps of Venus and Mars. The other 80%? The reality is that most of our oceans are totally untouched. Even though 70% of Earth is covered by oceans, we know little about our ocean seafloor.
Despite the need to understand ocean CO2 sequestration, nutrient recycling and untapped energy resources, the biggest drawback is the high cost of exploring oceans.
79 The Earth is breathing
Net primary productivity is how much carbon dioxide is taken in during photosynthesis minus how much is given off during respiration.
For example, lush tropical rainforests are the most productive places on the planet. But tundras are least productive because little photosynthesis takes place in polar regions.
80 Climate feedback loops
Because clouds reflect ⅓ of incoming solar radiation, more clouds could slow the increased warming from less heat absorption. This is an example of a negative feedback loop. An example of a positive feedback loop is the melting of permafrost.
This amplifies climate change because its methane contents would be released into the atmosphere.
81 Watersheds are like upside down umbrellas
Think of a watershed like an upside-down umbrella. The canopy catches water to eventually end up at the lowest depression.
These depressions are often well-connected networks of tributaries. They zig-zag all the way to a main body of water like a river or lake. That means everything upstream ends up downstream.
82 Salinity in oceans
When ocean evaporates from heat, salt remains in the ocean and water rises. Even though rain water wakes minerals and salts into rivers and lakes, they are mostly freshwater.
This is because their minerals get washed away and transported to an outlet at the nearest ocean. So unlike the high salinity we find in oceans, lakes and rivers constantly have the minerals washed away.
83 Deltas are fertile and often overcrowded
At this point, the stream loses energy because of the increased sediment deposits. This forces the basin entrance to widen forming a delta. Deltas take different shapes.
If you have too much sediment deposits, a feature like a bird-foot delta forms. When it floods, sediments spread across the region. When water recedes, soils are rich and fertile for agriculture purposes.
84 Soil formation from weathering
That’s why from top to bottom, soils get rockier further down. But other types of weathering can peel away at rock as soil formation factors.
Most importantly, soil differs geographically. For example, tropical rainforests have a thick pedosphere because of the abundance of rain in this region.
85 The Nitrogen cycle from the air to soil
When bacteria in the soil takes nitrogen from the air, it becomes nitrates and can move through the food chain. For example, legumes like clovers, peas and beans, their roots can take N2 from the air and transform into another form called nitrates.
In addition, lightning transforms N2 into NO2, which goes into the soil to form nitrates. Also, synthetic fertilizer from farming can bring nitrate to the soil.
86 Lighting strikes 8.6 million times per day.
You get a shock because you discharge the static electric charge to a positively charged object. Similarly, lightning is an electrostatic discharge that is supercharged from ionized air.
Lightning always finds the fastest route to Earth. By releasing a massive bolt of electricity, lightning is hotter than the sun when it strikes. Lightning strikes 8.6 million times a day. It helps in the production of ozone and nitrogen fixation.
87 Nutrient cycle – From inorganic to organic
Because Earth is a closed system, nothing is taken out or in. It’s just recycled back and forth. First, plants uptake nutrients from the soil to grow. Then, animals consume plants and make waste. Eventually, plants die and decay becoming litter in the soil.
Decomposers break it down where it can be recycled to be part of the food chain again. This vital process releases nutrients and replenishes the soil keeping the nutrient cycle in balance. This process of production and decomposition is deep-rooted and is the life blood in fully functional ecosystems.
88 Nutrient-deprived soils
If you deplete the soil from these nutrients, this deprives the plants from growing. For example, this is an ongoing problem for farming and tree harvesting areas.
This is why farmers rotate crops and allow periods of rest or “fallow” to replenish soil with nutrients. In addition, farmers use chemical and natural fertilizers to replace nitrogen which are leached from the soil by growing plants or runoff into streams.
89 Koppen climate classification
In the eyes of Koppen, Earth consists of 5 climate types – tropical, dry, temperate, continental and polar. Dry climates are characterized by having a shortage of water.
While polar climates endure frigid temperatures (-10 °C), tropical climates sustain a healthy portion of high temperature (+18 °C). Temperate climates take the middle road for average temperature. Finally, continental climates are usually situated in the interior of continents.
90 Resilient ecosystems from biodiversity
A loss in biodiversity is like a soccer team without a defense. If you lose specific habitats like wetlands, grasslands and forests, then you threaten biodiversity. It’s from the richness in species that we can derive certain pharmaceutical products.
For example, 1/4 of drugs we commonly use today were originally derived from plants. Most of these were discovered in rainforests where biodiversity is immense.
91 Coral reefs as biodiversity hotspots
These are like the rainforests of the oceans. From an environmental standpoint, there’s been a race to protect them. Not only does overfishing threaten coral reef health, but stress from rising temperature, ocean acidity even sunscreen can harm coral reef.
Scientists argue that coral reefs face extinction in 50 years. So the spotlight is on coral reef. For example, replanting is just one way scientists are restoring these underwater biodiversity hotspots.
92 The food chain and you
At the bottom of the food chain, plants are natural producers and provide food and nutrients to consumers. Herbivores nourish on plants and insects. Then, predators prey on herbivores or other predators.
When an animal dies, scavengers and decomposers break them down. Afterwards, it can be recycled to be part of the food chain again.
93 Your body is 90% bacteria
Bacteria are instrumental in breaking down sugars, digesting food and protect against infections. And the reason is because your body functions best by evolving with both human cells and bacteria.
You wouldn’t be who are you today if it wasn’t for the underappreciated bacteria.
94 Humans have existed for <1% of Earth's history
The earliest modern human fossil found was dated to be about 200,000 years old. Humans migrated and spread throughout the continents.
Like an insurance policy, this helped prevent humans from extinction during cold spells. But our distinct advantage was our enormous brains and ability to communicate.
95 We are made of stardust
This is the dying last stage of a star when the star explodes. Heavier elements like copper and zinc get flung out into space. We find these elements in our bodies and the food we eat.
So that means we are composed of bits of old supernova and cosmic dust.
96 Energy conversion through cellular respiration
From glucose and oxygen, cellular respiration is the mechanism that gives us the energy we need to live.
All the chemical reactions in living things run off ATP. Basically, sugars, fats and proteins turn into ATP which is the usable form of energy for biological systems like ours.
97 7.6 billion humans live on Earth and counting
We customize our environment by erecting cities, chopping down forests and altering the chemical makeup of the atmosphere.
Unequivocally, humans are transforming the landscape at an unsustainable rate.
98 The greatest gift for your children
Like a one-man wrecking ball, humans emit methane, carbon dioxide and aerosol greenhouse gases. These are the heavy hitters which continue to fill the air at unprecedented rates.
Overall, we need a new strategy. Not wishful thinking.
99 Sea levels constantly change
Scientists estimate sea level will rise 32 to 68 inches by 2100. This rise in sea levels could swallow parts of coastal cities like Shanghai, Olympia and New York. How do we slow down the massive supply of water?
First, we reverse deforestation to capture more carbon from the atmosphere. Second, we reduce greenhouse gas emissions to help stabilize temperature. Finally, we all have to consider the environment in our daily lives.
100 Earth will be fine.
Eventually, continental drift will assemble another supercontinent called Pangaea Ultima. The universe’s age is 13.7 billion years ago. Stars will continue to form for another 100 trillion years.
We talk about terraforming Mars. But we can’t even take care of our own. In a game of cat and mouse, the clock is ticking. Just like 99% of species that ever existed, we’re not extinction proof. Earth will be fine. But we won’t.