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the claim
Earth's life depends on its precise distance from the sun
the verdict
INSUFFICIENT LEANING
refutedsupported
the weight of evidence
5 sources for · 0 against

The counted sources provide background on Earth and planetary conditions, but they do not provide sufficient support for the claim that Earth's life depends on its precise distance from the sun.

Evidence for · 5
cited by 0
Earth is the third planet from the Sun and the only astronomical object known to harbor life. This is made possible by Earth being an ocean world, the only one in the Solar System sustaining liquid surface water. Almost all of Earth's water is contained in its ocean, which covers 70.8% of Earth's crust. The remaining 29.2% of Earth's crust is land, which is predominantly located within Earth's lan Earth is the third planet from the Sun and the only astronomical object known to harbor life. This is made possible by Earth being an ocean world, the only one in the Solar System sustaining liquid surface water. Almost all of Earth's water is contained in its ocean, which covers 70.8% of Earth's crust. The remaining 29.2% of Earth's crust is land, which is predominantly located within Earth's land hemisphere in the form of continental landmasses. Most of Earth's land is at least somewhat humid and covered by vegetation, while large ice sheets at Earth's polar deserts retain more water than Earth's groundwater, lakes, rivers, and atmospheric water combined. Earth's crust consists of slowly moving tectonic plates, which interact to produce mountain ranges, volcanoes, and earthquakes. Earth has a liquid outer core that generates a magnetosphere capable of deflecting most of the destructive solar winds and cosmic radiation. Earth has a dynamic atmosphere, which sustains Earth's surface conditions and protects it from most meteoroids and ultraviolet light at entry. It is composed primarily of nitrogen and oxygen. Water vapor is widely present in the atmosphere, forming clouds that cover most of the planet. The water vapor acts as a greenhouse gas and, together with other greenhouse gases in the atmosphere, particularly carbon dioxide (CO2), creates the conditions for both liquid surface water and water vapor to persist via the capturing of energy from the Sun's light. This process maintains the current average surface temperature of 14.76 °C (58.57 °F), at which water is liqu Earth is the third planet from the Sun and the only astronomical object known to harbor life. This is made possible by Earth being an ocean world, the only one in the Solar System sustaining liquid surface water. Almost all of Earth's water is contained in its ocean, which covers 70.8% of Earth's crust. The remaining 29.2% of Earth's crust is land, which is predominantly located within Earth's land hemisphere in the form of continental landmasses. Most of Earth's land is at least somewhat humid and covered by vegetation, while large ice sheets at Earth's polar deserts retain more water than Earth's groundwater, lakes, rivers, and atmospheric water combined. Earth's crust consists of slowly moving tectonic plates, which interact to produce mountain ranges, volcanoes, and earthquakes. Earth has a liquid outer core that generates a magnetosphere capable of deflecting most of the destructive solar winds and cosmic radiation. Earth has a dynamic atmosphere, which sustains Earth's surface conditions and protects it from most meteoroids and ultraviolet light at entry. It is composed primarily of nitrogen and oxygen. Water vapor is widely present in the atmosphere, forming clouds that cover most of the planet. The water vapor acts as a greenhouse gas and, together with other greenhouse gases in the atmosphere, particularly carbon dioxide (CO2), creates the conditions for both liquid surface water and water vapor to persist via the capturing of energy from the Sun's light. This process maintains the current average surface temperature of 14.76 °C (58.57 °F), at which water is liquid under normal atmospheric pressure. Differences in the amount of captured energy between geographic regions (as with the equatorial region receiving more sunlight than the polar regions) drive atmospheric and ocean currents, producing a global climate system with different climate regions, and a range of weather phenomena such as precipitation, allowing components such as carbon and nitrogen to cycle. Earth is rounded into an ellipsoid with a circumference of about 40,000 kilometres (24,900 miles). It is the densest planet in the Solar System. Of the four rocky planets, it is the largest and most massive. Overall, Earth is the sixth largest object in the Solar System after the Sun and the outer planets. Earth is about eight light-minutes (1 AU) away from the Sun and orbits it, taking a year (about 365.25 days) to complete one revolution. Earth rotates around its own axis in slightly less than a day (in about 23 hours and 56 minutes). Earth's axis of rotation is tilted with respect to the perpendicular to its orbital plane around the Sun, producing seasons. Earth is orbited by one permanent natural satellite, the Moon, which orbits Earth at 384,400 km (238,855 mi)—1.28 light seconds—and is roughly a quarter as wide as Earth. The Moon's gravity helps stabilize Earth's axis, causes tides and gradually slows Earth's rotation. Likewise, Earth's gravitational pull has already made the Moon's rotation tidally locked, keeping the same near side facing Earth. Earth, like most other bodies in the Solar System, formed about 4.5 billion years ago from gas and dust in the early Solar System. The formation of the ocean and the subsequent development of life occurred during the first billion years of Earth's history. Life spread globally and has been altering Earth's atmosphere and surface, leading to the Great Oxidation Event two billion years ago. Humans emerged 300,000 years ago in Africa and have spread across every continent on Earth. Humans depend on Earth's biosphere and natural resources for their survival, but have increasingly impacted the planet's environment. Humanity's current impact on Earth's climate and biosphere is unsustainable, threatening the livelihood of humans and many other forms of life, and causing widespread extinctions. The gravity of Earth is the acceleration that is imparted to objects due to the distribution of mass within Earth. Near
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More for · 4
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Habitable zones with an earth climate history model - ScienceDirect Skip to main contentSkip to article - Access through your organization - Purchase PDF Search ScienceDirect ## Planetary and Space Science Volume 206, 15 October 2021, 105318 # Habitable zones with an earth climate history model Barton Paul Levenson Show more Add to Mendeley https://doi.org/10.1016/j.pss.2021.105318 Get rights and content ## Highlights • Earth's climate was simulated across geological time. • Seafloor weathering is less sensitive to temperature than continental. • This makes Earth's carbonate-silicate cycle a less effective climate feedback. • It exposes Earth to limit cycling at the habitable zone outer boundary. • This produces a narrower habitable zone around the sun. ## Introduction The idea of simulating Earth's climate throughout geological history was introduced by Hart (1978, 1979), and was attempted subsequently by, e.g., Franck et al. (2002) and Krissansen-Totton et al. (2018). Hart's model found a very narrow continuously habitable zone (CHZ) for the sun, from 0.958 to 1.004 AU. If we define the ratio of outer to inner boundary as the “spacing ratio” R, this gives
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What determines if a planet can have life? - NASA Science Search ## Suggested Searches Explore This Section # 3.3. What determines if a planet can have life? A core learning question from the Astrobiology Learning Progressions ## Astrobiology Learning Progressions Navigation ### Previous 3.2. What does life need for survival? ### Next 3.4. Why is water so important for life as we know it? ## Grades K-2 or Adult Naive Learner - Storyline - NGSS Connections for Teachers - Concept Boundaries for Scientists - Resources Do you know the story of Goldilocks and the Three Bears? Goldilocks thought the Papa Bear’s porridge was too hot and Mama Bear’s porridge was too cold and Baby Bear’s porridge was just right. That’s a great story but it’s also a good way to think of our home. Sometimes we can feel cold or hot but really most the time, it’s just right. When we think about our planet, the warmth that comes from the Sun keeps our world from being too cold. Earth is far enough from the Sun that it is not too hot for us to live. It’s just right. If a planet has habitable conditions, or environmental conditions in which life may survive, then life may have evolved there. These co
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ystem whose English name does not come from Greek or Roman mythology. The name was taken from Old English and Germanic. It simply means "the ground." There are, of course, many names for our planet in the thousands of languages spoken by the people of the third planet from the Sun. Unable to render the provided source Namesake The name Earth is about 1,000 years old. All of the planets, except for Earth, were named after Greek and Roman gods and goddesses. However, the name Earth is a Germanic word, which simply means “the ground.” Potential for Life Earth has a very hospitable temperature and mix of chemicals that have made life abundant here. Most notably, Earth is unique in that most of our planet is covered in liquid water, since the temperature allows liquid water to exist for extended periods of time. Earth's vast oceans provided a convenient place for life to begin about 3.8 billion years ago. Some of the features of our planet that make it great for sustaining life are changing due to the ongoing effects of climate change . Size and Distance With an equatorial diameter of 7,926 miles (12,756 kilometers), Earth is the biggest of the terrestrial planets and the fifth largest planet in our solar system. From an average distance of 93 million miles (150 million kilometers), Earth is exactly one astronomical unit away from the Sun because one astronomical unit (abbreviated as AU), is the distance from the Sun to Earth. This unit provides an easy way to quickly compare planets' distances from the Sun. It takes about eight minutes for light from the Sun to reach our planet. Orbit and Rotation As Earth orbits the Sun, it completes one rotation every 23.9 hours. It takes 365.25 days to complete one trip around the Sun. That extra quarter of a day presents a challenge to our calendar system, which counts one year as 365 days. To keep our yearly calendars consistent with our orbit around the Sun, every four years we add one day. That day is called a leap day, and the y
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Goodbye, Goldilocks? The untimely end of life on Earth | New Scientist # Goodbye, Goldilocks? The untimely end of life on Earth From life’s point of view, Earth sits in the solar system’s sweet spot. But new calculations suggest it is teetering on the brink of a solar roasting By Lee Billings 5 June 2013 Will things be “just right” for much longer?(Image: Sam Chivers) Editorial “ Is Earth’s orbit scarily close to Venus’s sultry zone?“ WE LIVE in the best of all possible worlds. This much-lampooned idea originated in the early 18th century, when the German polymath Gottfried Leibniz was pondering what sort of world a benevolent God would make. In the past couple of decades, however, it has acquired a new resonance as we have spied out worlds orbiting other stars. The question is whether any of these, too, might support life. Underpinning each assessment is a surprisingly simple process that measures each of our potential planetary twins – or, more likely, near cousins – against a presumed earthly idyll. To host life, a world must, like Earth, be rocky, watery and orbiting in a star’s “Goldilocks zone”, where things are not too hot, not too cold, but just right. But do we
Everything we examined (5) — 4 independent sources
This check searched the claim as stated. It did not run a separate search for evidence against it.
  1. Earthreferenceno side taken
  2. Habitable zones with an earth climate history model - ScienceDirectreferenceno side taken
  3. What determines if a planet can have life? - NASA Sciencereferencesame source L45no side taken
  4. Facts About Earthofficial-recordsame source L45no side taken
  5. Goodbye, Goldilocks? The untimely end of life on Earth | New Scientistnews-webno side taken
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