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Bumi

Wikipedia Minangkabau - Lubuak aka tapian ilimu
Bumi  🜨
"Pualam Biru" foto bumi,
diambiak dariApollo 17
Panamoan
Pangucapan/en-us-earth.oggˈɜrθ/
Istilahearthly, tellurian, telluric, terran, terrestrial.
Jangka wakatuJ2000.0[note 1]
Aphelion152,098,232 km
1.01671388 AU[note 2]
Perihelion147,098,290 km
0.98329134 AU[note 2]
Sumbu semi-mayor149,598,261 km
1.00000261 AU[1]
Eksentrisitas0.01671123[1]
Periode orbit365.256363004 days[2]
1.000017421 tahun
Kacapatan orbit rato-rato29.78 km/s[3]
107,200 km/h
Anomalirato-rato357.51716°[3]
Inklinasi7.155° dari equator Matohari
1.57869°[4] toinvariable plane
Bujua node manaiak348.73936°[3][note 3]
Argumen perihelion114.20783°[3][note 4]
Satelit1 natural (Bulan)
8,300+ artificial (pada1 Maret2001 (2001-03-01)[update])[5]
Karakteristik fisik
Jari-jari
rato-rato
6,371.0 km[6]
Jari-jari
ekuator
6,378.1 km[7][8]
Radiuskutub6,356.8 km[9]
Kapapatan0.0033528[10]
Kaliliang40,075.017 km (equatorial)[8]
40,007.86 km (meridional)[11]
Laweh pamukoan510,072,000 km2[12][13][note 5]

148,940,000 km2 land (29.2 %)

361,132,000 km2 water (70.8 %)
Volume1.08321×1012 km3[3]
Masso5.9736×1024 kg[3]
Masso jenis
rato-rato
5.515 g/cm3[3]
Gravitasi pamukoan ekuator9.780327m/s2[14]
0.99732 g
Kacapatan palapehan11.186 km/s[3]
Hari sideris0.99726968 d[15]
23h 56m 4.100s
Kacapatan rotasi1,674.4 km/h (465.1 m/s)[16]
Kamiriangan sumbu23°26'21".4119[2]
Albedo0.367 (geometric)[3]
0.306 (Bond)[3]
Suhu pamukoan
   Kelvin
   Celsius
minrato-ratomax
184 K[17]287.2 K[18]331 K[19]
-89.2 °C14 °C57.8 °C
Atmosfir
Takanan pamukoan101.325 kPa (MSL)
Komposisi78.08% Nitrogen (N2)[3]
20.95% oxygen (O2)
0.93% Argon
0.038% Karbon diosida
About 1%water vapor (varies withKlimak)

Bumi adolahplanet katigo darimatohari, dan marupoan planet nan tapadek jo gadang nan ka limo dari salapan planet ditata surya. Inyo ko juo tamasuak paliang gadang dari nan ampek buah planet terrestrial. Bumi ko dirujuak juo sabagaidunia, planet biru,[20] atau namolatinnyo,Terra.[note 6]

Bumi ko rumah bagi jutaanspesies, tamasuakmanusia, bumi kini ko manjadi satu-satunyobenda astronomi nan di situ adokehidupan.[21] Planet ko tabantuak4.54 billion taun lalu, dankehidupan muncul di permukaan bumi sekitar satu billion taun.[22] Adonyobiosfir di bumi nan signifikan maubahatmosfir dan kondisiabiotik lainnyo di bumi, mamungkinkan proliferasiorganisme aerobik sarato pambentukan lapisanozon, basamo jomedan magnet bumi, mahalangiradiasi matohari, sahinggo mamungkinkan adonyo kehidupan di darek.[23] Sacarogeofisik bumi, misalnyo sajarahgeologi dan orbit, mamungkinkan kehidupan lah batahan salamo periode ko. Planet ko dihrapakan dapek taruih batahan untuak mandukuang kehidupan satidaknyo sampai500 milyar taun lai.[24][25]

Kronologi

[suntiang |suntiang sumber]

Urang cadiak pandai kini lah mampu marekonstruksi ulang maklumat rinci tantang maso lalu planet ko. Penanggalan awal tabantuaknyo sistem surya ko4.5672 ± 0.0006 billion taun lalu,[26] atau 4.54 billion tahun lalu (1% indak pasti)[22] the Earth and the other planets in the Solar System had formed out of thesolar nebula—a disk-shaped mass of dust and gas left over from the formation of the Sun. This assembly of the Earth through accretion was thus largely completed within 10–20 million years.[27] Initiallymolten, the outer layer of the planet Earth cooled to form a solid crust when water began accumulating in the atmosphere. The Moon formed shortly thereafter,4.53 billion years ago.[28]

Catatan

[suntiang |suntiang sumber]
  1. All astronomical quantities vary, bothsecularly andperiodically. The quantities given are the values at the instant J2000.0 of the secular variation, ignoring all periodic variations.
  2. abaphelion =a × (1 +e); perihelion =a × (1 -e), wherea is the semi-major axis ande is the eccentricity.
  3. The reference lists the longitude of the ascending node as -11.26064°, which is equivalent to 348.73936° by the fact that any angle is equal to itself plus 360°.
  4. The reference lists thelongitude of perihelion, which is the sum of the longitude of the ascending node and the argument of perihelion. That is, 114.20783° + (-11.26064°) = 102.94719°.
  5. Due to natural fluctuations, ambiguities surroundingice shelves, and mapping conventions forvertical datums, exact values for land and ocean coverage are not meaningful. Based on data from theVector Map andGlobal LandcoverArchived 2015-03-26 diWayback Machine. datasets, extreme values for coverage of lakes and streams are 0.6% and 1.0% of the Earth's surface. The ice shields ofAntarctica andGreenland are counted as land, even though much of the rock which supports them lies below sea level.
  6. ByInternational Astronomical Union convention, the termterra is used only for naming extensive land masses on celestial bodies other than the Earth.Cf.Blue, Jennifer (2007-07-05)."Descriptor Terms (Feature Types)".Gazetteer of Planetary Nomenclature. USGS. Diakses tanggal2007-07-05. 

Rujuakan

[suntiang |suntiang sumber]
  1. abStandish, E. Myles; Williams, James C."Orbital Ephemerides of the Sun, Moon, and Planets"(PDF). International Astronomical Union Commission 4: (Ephemerides). Diarsipkan dariversi asli(PDF) tanggal 2012-02-20. Diakses tanggal2010-04-03. Pemeliharaan CS1: Banyak nama: authors list (link) See table 8.10.2. Calculation based upon 1 AU = 149,597,870,700(3) m.
  2. abStaff (2007-08-07)."Useful Constants".International Earth Rotation and Reference Systems Service. Diakses tanggal2008-09-23. 
  3. abcdefghijkWilliams, David R. (2004-09-01)."Earth Fact Sheet". NASA. Diakses tanggal2010-08-09. 
  4. Allen, Clabon Walter; Cox, Arthur N. (2000). Allen's Astrophysical Quantities. Springer. p. 294. ISBN0-387-98746-0. http://books.google.com/?id=w8PK2XFLLH8C&pg=PA294. Diakses pado 13 Maret 2011. 
  5. US Space Command (March 1, 2001)."Reentry Assessment - US Space Command Fact Sheet". SpaceRef Interactive. Diakses tanggal2011-05-07. [pranala nonaktif permanen]
  6. Various (2000). David R. Lide. ed. Handbook of Chemistry and Physics (edisi ke-81st). CRC. ISBN0-8493-0481-4. 
  7. "Selected Astronomical Constants, 2011".The Astronomical Almanac. Diarsipkan dariversi asli tanggal 2013-08-26. Diakses tanggal2011-02-25. 
  8. abWorld Geodetic System (WGS-84).Available online fromNational Geospatial-Intelligence Agency.
  9. Cazenave, Anny (1995). "Geoid, Topography and Distribution of Landforms". di dalam Ahrens, Thomas J (PDF). Global earth physics a handbook of physical constants. Washington, DC: American Geophysical Union. ISBN0-87590-851-9. http://www.agu.org/reference/gephys/5_cazenave.pdf. Diakses pado 3 Agustus 2008. 
  10. IERS Working Groups (2003). "General Definitions and Numerical Standards". di dalam McCarthy, Dennis D.; Petit, Gérard. IERS Technical Note No. 32. U.S. Naval Observatory and Bureau International des Poids et Mesures. Diarsipan darinan asli pada 19 April 2014. https://web.archive.org/web/20140419043412/http://www.iers.org/MainDisp.csl?pid=46-25776. Diakses pado 3 Agustus 2008. 
  11. Humerfelt, Sigurd (October 26, 2010)."How WGS 84 defines Earth". Diakses tanggal2011-04-29. 
  12. Pidwirny, Michael (2006-02-02)."Surface area of our planet covered by oceans and continents.(Table 8o-1)". University of British Columbia, Okanagan. Diakses tanggal2007-11-26. 
  13. Staff (2008-07-24)."World".The World Factbook. Central Intelligence Agency. Diarsipkan dariversi asli tanggal 2010-01-05. Diakses tanggal2008-08-05. 
  14. Yoder, Charles F. (1995). T. J. Ahrens. ed. Global Earth Physics: A Handbook of Physical Constants. Washington: American Geophysical Union. p. 12. ISBN0-87590-851-9. http://www.agu.org/reference/gephys.html. Diakses pado 17 Maret 2007. 
  15. Allen, Clabon Walter; Cox, Arthur N. (2000). Allen's Astrophysical Quantities. Springer. p. 296. ISBN0-387-98746-0. http://books.google.com/?id=w8PK2XFLLH8C&pg=PA296. Diakses pado 17 Agustus 2010. 
  16. Arthur N. Cox, ed (2000). Allen's Astrophysical Quantities (edisi ke-4th). New York: AIP Press. p. 244. ISBN0-387-98746-0. http://books.google.com/?id=w8PK2XFLLH8C&pg=PA244. Diakses pado 17 Agustus 2010. 
  17. "World: Lowest Temperature".WMO Weather and Climate Extremes Archive. Arizona State University. Diarsipkan dariversi asli tanggal 2010-06-16. Diakses tanggal2010-08-07. 
  18. Kinver, Mark (December 10, 2009)."Global average temperature may hit record level in 2010".BBC Online. Diakses tanggal2010-04-22. 
  19. "World: Highest Temperature".WMO Weather and Climate Extremes Archive.Arizona State University. Diarsipkan dariversi asli tanggal 2013-01-04. Diakses tanggal2010-08-07. 
  20. Drinkwater, Mark; Kerr, Yann; Font, Jordi; Berger, Michael (February 2009)."Exploring the Water Cycle of the 'Blue Planet': The Soil Moisture and Ocean Salinity (SMOS) mission"(PDF).ESA Bulletin.European Space Agency (137): 6–15.A view of Earth, the ‘Blue Planet’ [...] When astronauts first went into the space, they looked back at our Earth for the first time, and called our home the ‘Blue Planet’. 
  21. May, Robert M. (1988). "How many species are there on earth?".Science.241 (4872): 1441–1449.Bibcode:1988Sci...241.1441M.doi:10.1126/science.241.4872.1441.PMID 17790039. 
  22. abSee:
  23. Harrison, Roy M. (2002). Causes and Environmental Implications of Increased UV-B Radiation. Royal Society of Chemistry. ISBN0-85404-265-2. 
  24. Britt, Robert (2000-02-25)."Freeze, Fry or Dry: How Long Has the Earth Got?". Archived from the original on 2009-06-05. Diakses tanggal2011-07-02. Pemeliharaan CS1: Url tak layak (link)
  25. Carrington, Damian (2000-02-21)."Date set for desert Earth". BBC News. Diakses tanggal2007-03-31. 
  26. Bowring, S. (1995). "The Earth's early evolution".Science.269 (5230): 1535.Bibcode:1995Sci...269.1535B.doi:10.1126/science.7667634.PMID 7667634. Parameter|coauthors= yang tidak diketahui mengabaikan (|author= yang disarankan) (bantuan)
  27. Yin, Qingzhu; Jacobsen, S. B.; Yamashita, K.; Blichert-Toft, J.; Télouk, P.; Albarède, F. (2002). "A short timescale for terrestrial planet formation from Hf-W chronometry of meteorites".Nature.418 (6901): 949–952.Bibcode:2002Natur.418..949Y.doi:10.1038/nature00995.PMID 12198540. 
  28. Kleine, Thorsten; Palme, Herbert; Mezger, Klaus; Halliday, Alex N. (2005-11-24). "Hf-W Chronometry of Lunar Metals and the Age and Early Differentiation of the Moon".Science.310 (5754): 1671–1674.Bibcode:2005Sci...310.1671K.doi:10.1126/science.1118842.PMID 16308422. Pemeliharaan CS1: Banyak nama: authors list (link)

Kepustakaan

[suntiang |suntiang sumber]

Pautan lua

[suntiang |suntiang sumber]
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