Venus: Difference between revisions

From WikiMD's Wellness Encyclopedia

CSV import
Tags: mobile edit mobile web edit
No edit summary
 
(One intermediate revision by the same user not shown)
Line 1: Line 1:
== Venus ==
[[File:Venus_2_Approach_Image.jpg|thumb|right|Approach image of Venus]]
[[File:Venus_2_Approach_Image.jpg|thumb|right|Approach image of Venus]]
 
[[File:Venus_symbol_(bold).svg|Symbol of Venus|thumb|left]]
[[File:Terrestrial_planet_size_comp_2024.png|Comparison of terrestrial planets|thumb|right]]
[[File:2438_pioneer_venus_map_of_venus.jpg|Map of Venus from Pioneer Venus|thumb|left]]
[[File:Venus_-_December_23_2016.png|Venus as seen in December 2016|thumb|right]]
[[File:Solar_system_orrery_inner_planets.gif|Orrery of inner planets|thumb|left]]
[[File:Venus_pentagram.png|Pentagram of Venus|thumb|right]]
'''Venus''' is the second planet from the [[Sun]] and is named after the Roman goddess of love and beauty. As the brightest natural object in the night sky after the [[Moon]], Venus can cast shadows and is often visible to the naked eye in broad daylight. Venus lies within [[Earth]]'s orbit, and so never appears to venture far from the Sun, either setting in the west just after dusk or rising in the east a bit before dawn. Venus orbits the Sun every 224.7 Earth days. With a rotation period of 243 Earth days, it takes longer to rotate about its axis than any other planet in the [[Solar System]] and does so in the opposite direction to most of the other planets.
'''Venus''' is the second planet from the [[Sun]] and is named after the Roman goddess of love and beauty. As the brightest natural object in the night sky after the [[Moon]], Venus can cast shadows and is often visible to the naked eye in broad daylight. Venus lies within [[Earth]]'s orbit, and so never appears to venture far from the Sun, either setting in the west just after dusk or rising in the east a bit before dawn. Venus orbits the Sun every 224.7 Earth days. With a rotation period of 243 Earth days, it takes longer to rotate about its axis than any other planet in the [[Solar System]] and does so in the opposite direction to most of the other planets.


Line 27: Line 30:
== Exploration ==
== Exploration ==
Venus has been explored by several spacecraft, including the Soviet Venera series, which provided the first images of the surface, and NASA's Magellan, which mapped the surface with radar. The European Space Agency's Venus Express orbited the planet from 2006 to 2014, studying its atmosphere and surface.
Venus has been explored by several spacecraft, including the Soviet Venera series, which provided the first images of the surface, and NASA's Magellan, which mapped the surface with radar. The European Space Agency's Venus Express orbited the planet from 2006 to 2014, studying its atmosphere and surface.
== Related pages ==
* [[Terrestrial planet]]
* [[Solar System]]
* [[Atmosphere of Venus]]
* [[Exploration of Venus]]
== References ==
* {{Cite book |last=Taylor |first=F. W. |title=The Scientific Exploration of Venus |year=2014 |publisher=Cambridge University Press |isbn=978-1-107-04354-5}}


== Gallery ==
== Gallery ==
<gallery>
<gallery>
File:Venus_symbol_(bold).svg|Symbol of Venus
File:Terrestrial_planet_size_comp_2024.png|Comparison of terrestrial planets
File:2438_pioneer_venus_map_of_venus.jpg|Map of Venus from Pioneer Venus
File:PIA00084_Eistla_region_pancake_volcanoes.jpg|Pancake volcanoes in Eistla region
File:PIA00103_Venus_-_3-D_Perspective_View_of_Lavinia_Planitia.jpg|3-D perspective view of Lavinia Planitia
File:Venus_-_December_23_2016.png|Venus as seen in December 2016
File:Solar_system_orrery_inner_planets.gif|Orrery of inner planets
File:Venus_pentagram.png|Pentagram of Venus
File:Venus-pacific-levelled.jpg|Venus over the Pacific
File:Venus-pacific-levelled.jpg|Venus over the Pacific
File:Lunar_Occultation_of_Venus_(NHQ201512070001).jpg|Lunar occultation of Venus
File:Lunar_Occultation_of_Venus_(NHQ201512070001).jpg|Lunar occultation of Venus
Line 53: Line 38:
File:Venus_Tablet_of_Ammisaduqa.jpg|Venus Tablet of Ammisaduqa
File:Venus_Tablet_of_Ammisaduqa.jpg|Venus Tablet of Ammisaduqa
File:Dresden_Codex_p09.jpg|Dresden Codex
File:Dresden_Codex_p09.jpg|Dresden Codex
File:Venus_Drawing.jpg|Drawing of Venus
File:Venus_Drawing.jpg|Drawing of Venus
File:Foto_de_Venera_9.png|Image from Venera 9
File:Foto_de_Venera_9.png|Image from Venera 9
Line 61: Line 45:
File:NASA_Cloud_City_on_Venus.jpg|Concept of a cloud city on Venus
File:NASA_Cloud_City_on_Venus.jpg|Concept of a cloud city on Venus
File:Kudurru_Melishipak_Louvre_Sb23_n02.jpg|Kudurru of Melishipak
File:Kudurru_Melishipak_Louvre_Sb23_n02.jpg|Kudurru of Melishipak
File:Van_Gogh_-_Starry_Night_-_Google_Art_Project.jpg|Venus in Van Gogh's Starry Night
</gallery>
</gallery>
== Related pages ==
* [[Terrestrial planet]]
* [[Solar System]]
* [[Atmosphere of Venus]]
* [[Exploration of Venus]]


[[Category:Venus]]
[[Category:Venus]]
[[Category:Terrestrial planets]]
[[Category:Terrestrial planets]]
[[Category:Solar System]]
[[Category:Solar System]]
==Venus==
'''Venus''' is the second planet from the [[Sun]] in our [[Solar System]]. It is named after the Roman goddess of love and beauty. Venus is often referred to as Earth's "sister planet" due to their similar size, composition, and proximity to the Sun.
==Physical Characteristics==
Venus is a [[terrestrial planet]] and is sometimes called Earth's "twin" because of their similar size and mass. However, the conditions on Venus are vastly different from those on Earth.
===Atmosphere===
The atmosphere of Venus is extremely dense and consists mainly of [[carbon dioxide]], with clouds of [[sulfuric acid]] droplets. The atmospheric pressure at the planet's surface is about 92 times that of Earth, which is equivalent to the pressure found 900 meters underwater on Earth.
===Surface===
The surface of Venus is covered with [[volcanoes]], large plains, and mountain ranges. The planet has more volcanoes than any other planet in the solar system, with over 1,600 major volcanoes. However, it is not known if any of these volcanoes are currently active.
===Temperature===
Venus is the hottest planet in the solar system, with surface temperatures reaching up to 467 degrees Celsius (872 degrees Fahrenheit). This extreme heat is due to a runaway [[greenhouse effect]] caused by the thick carbon dioxide atmosphere.
==Orbit and Rotation==
Venus orbits the Sun at an average distance of about 108 million kilometers (67 million miles). It takes Venus about 225 Earth days to complete one orbit around the Sun. However, Venus has a very slow rotation on its axis, taking about 243 Earth days to complete one rotation. Interestingly, Venus rotates in the opposite direction to most planets in the solar system, a phenomenon known as [[retrograde rotation]].
==Exploration==
Venus has been explored by several spacecraft, including the Soviet [[Venera]] program, which successfully landed probes on the planet's surface. The [[Magellan]] mission, launched by [[NASA]], mapped the surface of Venus using radar.
==Related Pages==
* [[Earth]]
* [[Mars]]
* [[Solar System]]
* [[Planetary Atmosphere]]
{{Solar System}}
[[Category:Planets]]
[[Category:Venus]]

Latest revision as of 04:07, 29 March 2025

Approach image of Venus
Symbol of Venus
Comparison of terrestrial planets
Map of Venus from Pioneer Venus
Venus as seen in December 2016
Orrery of inner planets
Pentagram of Venus

Venus is the second planet from the Sun and is named after the Roman goddess of love and beauty. As the brightest natural object in the night sky after the Moon, Venus can cast shadows and is often visible to the naked eye in broad daylight. Venus lies within Earth's orbit, and so never appears to venture far from the Sun, either setting in the west just after dusk or rising in the east a bit before dawn. Venus orbits the Sun every 224.7 Earth days. With a rotation period of 243 Earth days, it takes longer to rotate about its axis than any other planet in the Solar System and does so in the opposite direction to most of the other planets.

Physical characteristics[edit]

Internal structure[edit]

Diagram of Venus's internal structure

Venus is a terrestrial planet and is sometimes called Earth's "sister planet" because of their similar size, mass, proximity to the Sun, and bulk composition. However, it has a radically different atmosphere and surface conditions. Venus has a central iron core and a rocky mantle, similar to Earth.

Surface[edit]

Surface of Venus from Venera 13

The surface of Venus is covered with smooth, volcanic plains, with two large highland areas: Ishtar Terra and Aphrodite Terra. The planet's surface is obscured by an opaque layer of highly reflective clouds of sulfuric acid, preventing its surface from being seen from space in visible light.

Atmosphere[edit]

Venus has an extremely dense atmosphere composed mainly of carbon dioxide, with clouds of sulfuric acid droplets. The atmospheric pressure at the planet's surface is about 92 times that of Earth's, and the thick atmosphere traps heat in a runaway version of the greenhouse effect that warms Earth.

Orbit and rotation[edit]

Venus orbits the Sun at an average distance of about 108 million kilometers (about 0.7 AU) and completes an orbit every 224.7 Earth days. Unlike most planets in the Solar System, Venus rotates on its axis in a direction opposite to its orbital motion around the Sun. This means that on Venus, the Sun rises in the west and sets in the east.

Observation[edit]

Phases of Venus

Venus is the third-brightest natural object in the sky after the Sun and the Moon. It is often visible in the morning or evening sky and is sometimes referred to as the "Morning Star" or "Evening Star." Venus exhibits phases like those of the Moon, which can be observed with a telescope.

Exploration[edit]

Venus has been explored by several spacecraft, including the Soviet Venera series, which provided the first images of the surface, and NASA's Magellan, which mapped the surface with radar. The European Space Agency's Venus Express orbited the planet from 2006 to 2014, studying its atmosphere and surface.

Gallery[edit]

Related pages[edit]