• Study Resource
  • Explore
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Theme 7.2 -- The Complete Solar System
Theme 7.2 -- The Complete Solar System

Planetary Diversity - MIT Computer Science and Artificial
Planetary Diversity - MIT Computer Science and Artificial

Origin and Nature of Planetary Systems
Origin and Nature of Planetary Systems

... Introduction: While there is only one Solar System (the system of the star Sol), as of early April 2015, there are 1207 known extrasolar planetary systems with 1911 known planets (called extrasolar planets or exoplanets). Of these planetary systems 480 have two or more planets. In this activity, we ...
A Planetary System Around Our Nearest Star is Emerging
A Planetary System Around Our Nearest Star is Emerging

Navigating by the Stars
Navigating by the Stars

Slide 1
Slide 1

... they run out of nuclear fuel.. Typically 1,000 times the size of our solar system These Ten have names like Owl, the Cat's Eye, the Ghost of Jupiter, Ring. This glorious final phase in the life of a star lasts only about 10,000 ...
Which Objects Represent the Eight Planets in Our
Which Objects Represent the Eight Planets in Our

... new, scientifically accepted definition of the word, “planet”. According to these scientists, a planet must have three characteristics: a) It must orbit a Star (Sun) b) It must have enough mass for its self-gravity to form it into a spherical shape c) It must have “cleared” nearby objects away from ...
ASTR1010_HW06
ASTR1010_HW06

CO 2 Cycle
CO 2 Cycle

Extra-Solar Planets
Extra-Solar Planets

Extraterrestrial Life
Extraterrestrial Life

Phys 1830: Lecture 33 - University of Manitoba Physics Department
Phys 1830: Lecture 33 - University of Manitoba Physics Department

IMPORTANT HISTORICAL DATES AND EVENTS
IMPORTANT HISTORICAL DATES AND EVENTS

Presentation - The Stimulating Physics Network
Presentation - The Stimulating Physics Network

Scale Model of the Solar System
Scale Model of the Solar System

Exoplanets - An ESO/OPTICON/IAU summer school on modern
Exoplanets - An ESO/OPTICON/IAU summer school on modern

Possibilities for life elsewhere in the Solar System In our fifth
Possibilities for life elsewhere in the Solar System In our fifth

February 2007
February 2007

Astronomy 07 Life in the Universe Final Exam Test Bank Homework
Astronomy 07 Life in the Universe Final Exam Test Bank Homework

PSC101-lecture12
PSC101-lecture12

Three Media Reports by Carole Gallagher
Three Media Reports by Carole Gallagher

AST 301 Fall 2007 Review for Exam 3 This exam covers only
AST 301 Fall 2007 Review for Exam 3 This exam covers only

... evidence that they once did exist? Explain clearly why the terrestrial and jovian planets have such different properties in terms of the theory described in this chapter. The section on the discovery of extrasolar planets is one of the most exciting and evolving areas in astronomy at this time, so I ...
The Newtonian Revolution: The discovery of natural law
The Newtonian Revolution: The discovery of natural law

... decent quantitative model of the planets’ motion • It had the Earth at the center • It placed the planets Mercury and Venus carefully to match the observed angle offsets between the sun and these planets. • Accounted for retrograde motion with epicycles. Then needed to offset the center of epicycles ...
Habitability
Habitability

Habitability
Habitability

< 1 ... 22 23 24 25 26 27 28 29 30 ... 53 >

Circumstellar habitable zone



In astronomy and astrobiology, the circumstellar habitable zone (CHZ), or simply the habitable zone, is the region around a star within which planetary-mass objects with sufficient atmospheric pressure can support liquid water at their surfaces. The bounds of the CHZ are calculated using the known requirements of Earth's biosphere, its position in the Solar System and the amount of radiant energy it receives from the Sun. Due to the importance of liquid water to life as it exists on Earth, the nature of the CHZ and the objects within is believed to be instrumental in determining the scope and distribution of Earth-like extraterrestrial life and intelligence.The habitable zone is also called the Goldilocks zone, a metaphor of the children's fairy tale of Goldilocks and the Three Bears, in which a little girl chooses from sets of three items, ignoring the ones that are too extreme (large or small, hot or cold, etc.), and settling on the one in the middle, which is ""just right"".Since the concept was first presented in 1953, stars have been confirmed to possess a CHZ planet, including some systems that consist of multiple CHZ planets. Most such planets, being super-Earths or gas giants, are more massive than Earth, because such planets are easier to detect. On November 4, 2013, astronomers reported, based on Kepler data, that there could be as many as 40 billion Earth-sized planets orbiting in the habitable zones of Sun-like stars and red dwarfs in the Milky Way. 11 billion of these may be orbiting Sun-like stars. The nearest such planet may be 12 light-years away, according to the scientists. The CHZ is also of particular interest to the emerging field of habitability of natural satellites, because planetary-mass moons in the CHZ might outnumber planets.In subsequent decades, the CHZ concept began to be challenged as a primary criterion for life. Since the discovery of evidence for extraterrestrial liquid water, substantial quantities of it are now believed to occur outside the circumstellar habitable zone. Sustained by other energy sources, such as tidal heating or radioactive decay or pressurized by other non-atmospheric means, the basic conditions for water-dependent life may be found even in interstellar space, on rogue planets, or their moons. In addition, other circumstellar zones, where non-water solvents favorable to hypothetical life based on alternative biochemistries could exist in liquid form at the surface, have been proposed.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report