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Fayl Faylın tarixçəsi Faylın istifadəsi Faylın qlobal istifadəsi MetaməlumatlarBu TIF faylın JPG formatındakı bu görünüş

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

The four sides of Neptune (captured by the Hubble Space Telescope).tif
www.wikimedia.az-az.nina.azhttps://www.wikimedia.az-az.nina.az
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image
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.

Faylın orijinalı(2.250 × 2.474 piksel, fayl həcmi: 1,3 MB, MIME növü: image/tiff)

image
Bu fayl Vikianbarda yerləşir. Açıqlama səhifəsindəki məlumatlar aşağıda göstərilib.
Vikianbar azad lisenziyalı media anbarıdır. Siz də töhfə verə bilərsiniz.
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
image
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.

Faylın tarixçəsi

Faylın əvvəlki versiyasını görmək üçün gün/tarix bölməsindəki tarixlərə klikləyin.

Tarix/VaxtMiniatürÖlçülərİstifadəçiŞərh
hal-hazırkı11:01, 10 iyul 2012image2.250 × 2.474 (1,3 MB){{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

Metaməlumatlar

Bu faylda fotoaparat və ya skanerlə əlavə olunmuş məlumatlar var. Əgər fayl sonradan redaktə olunubsa, bəzi parametrlər bu şəkildə göstərilənlərdən fərqli ola bilər.

Genişlik2.250 px
Hündürlük2.474 px
Bits per component
  • 8
  • 8
  • 8
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.

wikipedia, oxu, kitab, kitabxana, axtar, tap, meqaleler, kitablar, oyrenmek, wiki, bilgi, tarix, tarixi, endir, indir, yukle, izlə, izle, mobil, telefon ucun, azeri, azəri, azerbaycanca, azərbaycanca, sayt, yüklə, pulsuz, pulsuz yüklə, haqqında, haqqinda, məlumat, melumat, mp3, video, mp4, 3gp, jpg, jpeg, gif, png, şəkil, muisiqi, mahnı, kino, film, kitab, oyun, oyunlar, android, ios, apple, samsung, iphone, pc, xiomi, xiaomi, redmi, honor, oppo, nokia, sonya, mi, web, computer, komputer

Fayl Faylin tarixcesi Faylin istifadesi Faylin qlobal istifadesi MetamelumatlarBu TIF faylin JPG formatindaki bu gorunusunun olcusu 545 599 piksel Diger olculer 218 240 piksel 436 480 piksel 698 768 piksel 931 1 024 piksel 2 250 2 474 piksel Faylin orijinali 2 250 2 474 piksel fayl hecmi 1 3 MB MIME novu image tiff Bu fayl Vikianbarda yerlesir Aciqlama sehifesindeki melumatlar asagida gosterilib Vikianbar azad lisenziyali media anbaridir Siz de tohfe vere bilersiniz IzahThe 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 Menbe http hubblesite org newscenter archive releases 2011 19 image a direct link Muellif NASA ESA and the Hubble Heritage Team STScI AURA Icaze Faylin tekrar istifadesi Public domain Public domain false false 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 Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtMiniaturOlculerIstifadeciSerh hal hazirki11 01 10 iyul 20122 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 039 s en Hubble Space Telescope ha Faylin istifadesi Asagidaki sehife bu fayli istifade edir Neptun planet Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur af wikipedia org layihesinde istifadesi Neptunus azb wikipedia org layihesinde istifadesi نپتون en wikipedia org layihesinde istifadesi Neptune en wikiversity org layihesinde istifadesi 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 layihesinde istifadesi Neptuun fr wikipedia org layihesinde istifadesi Neptune planete gl wikipedia org layihesinde istifadesi Neptuno id wikipedia org layihesinde istifadesi Neptunus ja wikipedia org layihesinde istifadesi 海王星 map bms wikipedia org layihesinde istifadesi Neptunus no wikipedia org layihesinde istifadesi Neptun planet ro wikipedia org layihesinde istifadesi Neptun vi wikipedia org layihesinde istifadesi Sao Hải VươngMetamelumatlar Bu faylda fotoaparat ve ya skanerle elave olunmus melumatlar var Eger fayl sonradan redakte olunubsa bezi parametrler bu sekilde gosterilenlerden ferqli ola biler Genislik2 250 pxHundurluk2 474 pxBits per component8 8 8SixilmamisLZWReng modeliRGBOrientasiyaNormalReng komponentlerinin sayi3Her blokdaki setirlerin sayi38Ufuqi xett300 dpiSaquli xett300 dpiData arrangementchunky formatProqram teminatiAdobe Photoshop CS5 MacintoshFaylin deyismesi tarixi ve vaxti10 07 11 iyul 2011Reng sahesisRGBwarningwrong data type 7 for RichTIFFIPTC tag ignored Menbe https az wikipedia org wiki Fayl The four sides of Neptune captured by the Hubble Space Telescope tif

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