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Fayl:The four sides of Neptune (captured by the Hubble Space Telescope).tif

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Fayl:The four sides of Neptune (captured by the Hubble Space Telescope).tif
Bu TIF-faylın JPG formatındakı bu görünüşünün ölçüsü: 545 × 599 piksel. Digər ölçülər: 218 × 240 piksel | 436 × 480 piksel | 698 × 768 piksel | 931 × 1.024 piksel | 2.250 × 2.474 piksel.

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İzahThe four sides of Neptune (captured by the Hubble Space Telescope).tif

On July 12, 2011, Neptune has arrived at the same location in space where it was discovered nearly 165 (Earth) years before (i.e. 1 Neptunian year). To commemorate the event, NASA's Hubble Space Telescope has taken these "anniversary pictures" of the blue-green giant planet.

Neptune is the most distant major planet in our solar system. German astronomer Johann Galle discovered the planet on September 23, 1846. At the time, the discovery doubled the size of the known solar system. The planet is 2.8 billion miles (4.5 billion kilometers) from the Sun, 30 times farther than Earth. Under the Sun's weak pull at that distance, Neptune plods along in its huge orbit, slowly completing one revolution approximately every 165 years.

These four Hubble images of Neptune were taken with the Wide Field Camera 3 on June 25-26, during the planet's 16-hour rotation. The snapshots were taken at roughly four-hour intervals, offering a full view of the planet. The images reveal high-altitude clouds in the northern and southern hemispheres. The clouds are composed of methane ice crystals.

The giant planet experiences seasons just as Earth does, because it is tilted 29 degrees, similar to Earth's 23-degree-tilt. Instead of lasting a few months, each of Neptune's seasons continues for about 40 years.

The snapshots show that Neptune has more clouds than a few years ago, when most of the clouds were in the southern hemisphere. These Hubble views reveal that the cloud activity is shifting to the northern hemisphere. It is early summer in the southern hemisphere and winter in the northern hemisphere.

In the Hubble images, absorption of red light by methane in Neptune's atmosphere gives the planet its distinctive aqua color. The clouds are tinted pink because they are reflecting near-infrared light.

A faint, dark band near the bottom of the southern hemisphere is probably caused by a decrease in the hazes in the atmosphere that scatter blue light. The band was imaged by NASA's Voyager 2 spacecraft in 1989, and may be tied to circumpolar circulation created by high-velocity winds in that region.

The temperature difference between Neptune's strong internal heat source and its frigid cloud tops, about minus 260 degrees Fahrenheit, might trigger instabilities in the atmosphere that drive large-scale weather changes.

Neptune has an intriguing history. It was Uranus that led astronomers to Neptune. Uranus, the seventh planet from the Sun, is Neptune's inner neighbor. British astronomer Sir William Herschel and his sister Caroline found Uranus in 1781, 55 years before Neptune was spotted. Shortly after the discovery, Herschel noticed that the orbit of Uranus did not match the predictions of Newton's theory of gravity. Studying Uranus in 1821, French astronomer Alexis Bouvard speculated that another planet was tugging on the giant planet, altering its motion.

Twenty years later, Urbain Le Verrier of France and John Couch Adams of England, who were mathematicians and astronomers, independently predicted the location of the mystery planet by measuring how the gravity of a hypothetical unseen object could affect Uranus's path. Le Verrier sent a note describing his predicted location of the new planet to the German astronomer Johann Gottfried Galle at the Berlin Observatory. Over the course of two nights in 1846, Galle found and identified Neptune as a planet, less than a degree from Le Verrier's predicted position. The discovery was hailed as a major success for Newton's theory of gravity and the understanding of the universe.

Galle was not the first to see Neptune. In December 1612, while observing Jupiter and its moons with his handmade telescope, astronomer Galileo Galilei recorded Neptune in his notebook, but as a star. More than a month later, in January 1613, he noted that the "star" appeared to have moved relative to other stars. But Galileo never identified Neptune as a planet, and apparently did not follow up those observations, so he failed to be credited with the discovery.

Neptune is not visible to the naked eye, but may be seen in binoculars or a small telescope. It can be found in the constellation Aquarius, close to the boundary with Capricorn.

Neptune-mass planets orbiting other stars may be common in our Milky Way galaxy. NASA's Kepler mission, launched in 2009 to hunt for Earth-size planets, is finding increasingly smaller extrasolar planets, including many the size of Neptune.
Tarix 25 iyun 2011 - 26 iyun 2011
date QS:P,+2011-06-00T00:00:00Z/10,P1319,+2011-06-25T00:00:00Z/11,P1326,+2011-06-26T00:00:00Z/11
Mənbə http://hubblesite.org/newscenter/archive/releases/2011/19/image/a/ (direct link)
Müəllif NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
İcazə
(Faylın təkrar istifadəsi)
Public domainPublic domainfalsefalse
Public domain
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.

The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.

For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.

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Tarix/VaxtMiniatürÖlçülərİstifadəçiŞərh
hal-hazırkı11:01, 10 iyul 201211:01, 10 iyul 2012 tarixindəki versiyanın miniatür görüntüsü2.250 × 2.474 (1,3 MB)Prof. Professorson{{Information |Description=On July 12, 2011, en:Neptune has arrived at the same location in space where it was discovered nearly 165 (Earth) years before (i.e. 1 Neptunian year). To commemorate the event, NASA's en:Hubble Space Telescope ha...

Faylın istifadəsi

Aşağıdakı səhifə bu faylı istifadə edir:

  • Neptun (planet)

Faylın qlobal istifadəsi

Bu fayl aşağıdakı vikilərdə istifadə olunur:

  • af.wikipedia.org layihəsində istifadəsi
    • Neptunus
  • azb.wikipedia.org layihəsində istifadəsi
    • نپتون
  • en.wikipedia.org layihəsində istifadəsi
    • Neptune
  • en.wikiversity.org layihəsində istifadəsi
    • User:Marshallsumter/Radiation astronomy/Cyans
    • User:Marshallsumter/Radiation astronomy1/Infrareds
    • Gases/Gaseous objects/Neptune
    • User:Marshallsumter/Radiation astronomy/Aerometeors
    • User:Marshallsumter/Radiation astronomy/Atmospheres
  • et.wikipedia.org layihəsində istifadəsi
    • Neptuun
  • fr.wikipedia.org layihəsində istifadəsi
    • Neptune (planète)
  • gl.wikipedia.org layihəsində istifadəsi
    • Neptuno
  • id.wikipedia.org layihəsində istifadəsi
    • Neptunus
  • ja.wikipedia.org layihəsində istifadəsi
    • 海王星
  • map-bms.wikipedia.org layihəsində istifadəsi
    • Neptunus
  • no.wikipedia.org layihəsində istifadəsi
    • Neptun (planet)
  • ro.wikipedia.org layihəsində istifadəsi
    • Neptun
  • vi.wikipedia.org layihəsində istifadəsi
    • Sao Hải Vương

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Genişlik2.250 px
Hündürlük2.474 px
Bits per component
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SıxılmamışLZW
Rəng modeliRGB
OrientasiyaNormal
Rəng komponentlərinin sayı3
Hər blokdakı sətirlərin sayı38
Üfüqi xətt300 dpi
Şaquli xətt300 dpi
Data arrangementchunky format
Proqram təminatıAdobe Photoshop CS5 Macintosh
Faylın dəyişməsi tarixi və vaxtı10:07, 11 iyul 2011
Rəng sahəsisRGB
warningwrong data type 7 for "RichTIFFIPTC"; tag ignored.
Mənbə — "https://az.wikipedia.org/wiki/Fayl:The_four_sides_of_Neptune_(captured_by_the_Hubble_Space_Telescope).tif"
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