cyanic-selkie/wikianc huggingface dataset:
Tẹ́lískópù Òfurufú Hubble
Pipeline reduction
Astronomical data taken with CCDs must undergo several calibration steps before they are suitable for astronomical analysis. STScI has developed sophisticated software that automatically calibrates data when they are requested from the archive using the best calibration files available. This 'on-the-fly' processing means that large data requests can take a day or more to be processed and returned. The process by which data are calibrated automatically is known as 'pipeline reduction', and is increasingly common at major observatories. Astronomers may if they wish retrieve the calibration files themselves and run the pipeline reduction software locally. This may be desirable when calibration files other than those selected automatically need to be used.
Data analysis
Hubble data can be analysed using many different packages. STScI maintains the custom-made STSDAS (Space Telescope Science Data Analysis System) software, which contains all the programs needed to run pipeline reduction on raw data files, as well as many other astronomical image processing tools, tailored to the requirements of Hubble data. The software runs as a module of IRAF, a popular astronomical data reduction program.
Outreach activities
It has always been important for the Space Telescope to capture the public's imagination, given the considerable contribution of taxpayers to its construction and operational costs. After the difficult early years when the faulty mirror severely dented Hubble's reputation with the public, the first servicing mission allowed its rehabilitation as the corrected optics produced numerous remarkable images.
Several initiatives have helped to keep the public informed about Hubble activities. The Hubble Heritage Project was established to provide the public with high-quality images of the most interesting and striking objects observed. The Heritage team is composed of amateur and professional astronomers, as well as people with backgrounds outside astronomy, and emphasizes the aesthetic nature of Hubble images. The Heritage Project is granted a small amount of time to observe objects which, for scientific reasons, may not have images taken at enough wavelengths to construct a full-color image.
STScI maintains several comprehensive websites for the general public containing Hubble images and information about the observatory. The outreach efforts are coordinated by the Office for Public Outreach, which was established in 2000 to ensure that US taxpayers saw the benefits of their investment in the space telescope program.
Since 1999, the leading Hubble outreach group in Europe has been the Hubble European Space Agency Information Centre (HEIC). This office was established at the Space Telescope - European Coordinating Facility in Munich, Germany. HEIC's mission is to fulfill HST outreach and education tasks for the European Space Agency. The work is centered on the production of news and photo releases that highlight interesting Hubble results and images. These are often European in origin, and so increase awareness of both ESA’s Hubble share (15%) and the contribution of European scientists to the observatory. ESA produces innovative educational material, including a videocast series called Hubblecast designed to share world-class scientific news with the public.
The Hubble Space Telescope has won two Space Achievement Awards from the Space Foundation for its outreach activities, in 2001 and 2010.
There is a replica of the Hubble Telescope on the courthouse lawn in Marshfield, Missouri, the hometown of namesake Edwin P. Hubble.
Equipment failure
Past servicing missions have exchanged old instruments for new ones, both avoiding failure and making possible new types of science. Without servicing missions, all of the instruments will eventually fail. In August 2004, the power system of the Space Telescope Imaging Spectrograph (STIS) failed, rendering the instrument inoperable. The electronics had originally been fully redundant, but the first set of electronics failed in May 2001. This power supply was fixed during servicing mission 4 in May 2009. Similarly, the main camera (the ACS) primary electronics failed in June 2006, and the power supply for the backup electronics failed on January 27, 2007. Only the instrument's Solar Blind Channel (SBC) was operable using the side-1 electronics. A new power supply for the wide angle channel was added during SM 4, but quick tests revealed this did not help the high resolution channel.
HST uses gyroscopes to stabilize itself in orbit and point accurately and steadily at astronomical targets. Normally, three gyroscopes are required for operation; observations are still possible with two, but the area of sky that can be viewed would be somewhat restricted, and observations requiring very accurate pointing are more difficult. There are further contingency plans for observations with just one gyro, but if all gyros fail, continued scientific observations will not be possible. In 2005, it was decided to switch to two-gyroscope mode for regular telescope operations as a means of extending the lifetime of the mission. The switch to this mode was made in August 2005, leaving Hubble with two gyroscopes in use, two on backup, and two inoperable. One more gyro failed in 2007. By the time of the final repair mission, during which all six gyros were replaced (with two new pairs and one refurbished pair), only three gyros were still working. Engineers are confident that they have identified the root causes of the gyro failures, and the new models should be much more reliable.
Orbital decay
Hubble orbits the Earth in the extremely tenuous upper atmosphere, and over time its orbit decays due to drag. If it is not re-boosted by a shuttle or other means, it will re-enter the Earth's atmosphere sometime between 2019 and 2032, with the exact date depending on how active the Sun is and its impact on the upper atmosphere. If Hubble were to descend in a completely uncontrolled re-entry, parts of the main mirror and its support structure would probably survive, leaving the potential for damage or even human fatalities.
NASA's original plan for safely de-orbiting Hubble was to retrieve it using a space shuttle. The Hubble telescope would then have most likely been displayed in the Smithsonian Institution. This is no longer possible since the space shuttle fleet has been retired, and would have been unlikely in any case due to the cost of the mission and risk to the crew. Instead NASA considered adding an external propulsion module to allow controlled re-entry. Ultimately NASA installed the Soft Capture and Rendezvous System, to enable retrieval by either a crewed or robotic mission.
Successors
There is no direct successor to the Hubble as an ultraviolet and visible-light space telescope, as near-term space telescopes do not duplicate Hubble's wavelength coverage (near-ultraviolet to near-infrared wavelengths), instead concentrating on the farther infrared bands. These bands are preferred for studying high redshift and low-temperature objects, objects generally older and farther away in the universe. These wavelengths are also difficult or impossible to study from the ground, justifying the expense of a space-based telescope. Large ground-based telescopes can image some of the same wavelengths as Hubble, sometimes challenge HST in terms of resolution (via adaptive optics), have much larger light-gathering power, and can be upgraded more easily, but cannot yet match the Hubble's excellent resolution over a wide field of view with the very dark background of space.
A complementary telescope, looking at even longer wavelengths than Hubble or JWST, is the European Space Agency's Herschel Space Observatory, launched on May 14, 2009. Like JWST, Herschel is not designed to be serviced after launch, and has a mirror substantially larger than Hubble's, but observes only in the far infrared.
Further concepts for advanced 21st-century space telescopes include the Advanced Technology Large-Aperture Space Telescope. , a conceptualized 8- to 16-meter (320- to 640-inch) optical space telescope that if realized could be a more direct successor to HST, with the ability to observe and photograph astronomical objects in the visible, ultraviolet, and infrared wavelengths, with substantially better resolution than Hubble or the Spitzer Space telescope. This effort is being planned for the 2025–2035 time frame.
Existing ground-based telescopes, and various proposed Extremely Large Telescopes, can exceed the HST in terms of sheer light-gathering power and diffraction limit due to larger mirrors, but other factors affect telescopes. In some cases, they may be able to match or beat Hubble in resolution by using adaptive optics (AO). However, AO on large ground-based reflectors will not make Hubble and other space telescopes obsolete. Most AO systems sharpen the view over a very narrow field—Lucky Cam, for example, produces crisp images just 10" to 20" wide, whereas Hubble's cameras are super sharp across a 2½' (150") field. Furthermore, space telescopes can study the heavens across the entire electromagnetic spectrum, most of which is blocked by Earth's atmosphere. Finally, the background sky is darker in space than on the ground, because air absorbs solar energy during the day and then releases it at night, producing a faint—but nevertheless discernible—airglow that washes out low-contrast astronomical objects.
Olódùmarè
Olódùmarè Káàkìri àgbáyé ni a ti mò pé olódùmarè wà, eni tí ó dá ayé àti òrùn àti ohun gbogbo ti ń be nínú won òyígíyigí oba àìrí arínú-róde Olùmòràn Òkàn, alèwílèse, alèselèwí, Oba atélè bí eni téní, Oba atésánmo bí eni téso, Oba lónìí, Oba lóla, Oba títí ayé àìnípèkun, Olówó gbogbogbo tí ń yomo rè nínú òfin, Oba Olójú lu kára bí ajere, Oba onínú fúnfún àti béè béè lo.
Èyí ni pe oríkì Olódùmarè pọ̀ lọ jáǹtìrẹrẹ, bí a bá sì gbọ́ tí àwọn Yorùbá bá sọ pé ‘orí mi o tàbí olọ́jọ́ ọ̀ní o, Olódùmarè ni wọ́n ń pè ní orí, èyí tí ó dúró fún ẹlẹda orí àti ọlọ́jọ́ òní tí ó dúró fún ẹ̀ni tí ó nì ọjọ́ òní. Tàbí nígbà mìíràn tí àwọn Yorùbá bá rí Ohun tí ó ya ni lẹ́nu wọn á ní ‘Bàbá ò’ èyí tí ó dúró fún Olódùmarè.
Bí a bá tún gbó nígbà mìíràn tí àwọn àgbàlagbà ń lo àwọn ọ̀rọ̀ bíi ‘Èdùàrè tàbí wọ́n ń lo àwọn ọ̀rọ̀ bíi ‘olú’ olódùmarè kan náà ni wọn ń tọ́ka sí. Àwọn àgbàlagbà a máa sọ pé:
“Àṣegbé ọmọ Èdùàrè
mo ló dàṣegbé
Àṣegbé ọmọ Èdùàrè…
Ohun tí àkọlé yìí ń tọ́ka sí ni pé ohun tí ọmọ Èdùàrè, èyí tí ó dúró fún olódùmarè bá ti ṣe àṣegbé ni ìgbà gbogbo là ń gbọ́ tí àwọn àgbàlagbà máa ń sọ pé “ẹni olúwa dá kò ṣe é fara wé”. Ohun tí wọn ń tọ́ka sí nínú gbólóhùn yìí nip é ẹni tí Olú, èyí tí ó dúró fún olódùmarè “bá ti dá àyànmọ́ kan mọ́ ẹnìkan, a kò lè fara wé irú ẹ̀nìyàn bẹ́ẹ̀.
Àwọn àkíyèsí tí a lè rí tọ́ka sí ni pé ọ̀pọ̀ ìtàn ìwásẹ̀ ni ó sọ bí Olódùmarè ṣe sẹ̀dá ayé àti ọ̀run, Yorùbá gbàgbọ́ pé ọ̀run ni olódùmarè wà, tí ó ti ń ṣe àkóso ayé àti ọ̀run, èrò Yorùbá ni pé kò sí ohun tí a ‘lè fi wé olódùmarè nítorí àwọn àwẹ̀mọ́ tàbí abuda rẹ tó tayọ àwa ẹ̀dá lọ fún àpẹẹrẹ a lè pe olódùmarè báyìí pé ‘Ẹlẹda, Ẹlẹ́mìí, Ọlọ́run Ọba ní í fọ́n èjí iwọ́rọ́ iwọ́rọ̣́, òun ló ni ọ̀sán àti òru dọ́jọ́ òní, òní ọmọ Ọlọ́fin, Ọ̀la ọmọ Ọlọ́fin, Ọ̀tunla ọmọ Ọlọ́fin, ìrènì ọmọ Ọlọ́fin, ọ̀rúnní ọmọ Ọlọ́fin, Yorùbá máa ń sọ pé ìṣẹ́ Ọlọ́run tóbi tàbí àwámárìdí ni iṣẹ́ Ọlọ́run, Ọ̀rúnmìlà fẹ̀yìntì ó wò títí o ní “ẹ̀yín èrò okun, ẹ̀yin èrò ọsa, ǹ jẹ́ ẹ̀yin ò mọ̀ pé iṣẹ́ Olódùmarè tóbi: A tún lè sọ pé Ọba Ọ̀run ọ̀gá Ògo, atẹ́rẹrẹ káyé ẹlẹ́ní àtẹ́ẹ̀ká, Ọba ti ọ̀rọ̀ rẹ̀ kì í yẹ̀, alábà láṣẹ̀ á tun le pe ni alágbára láyé àti lọ́run.
Adùn ún ṣe bí ohun tí olódùmarè lọ́wọ́ sí, aṣòro o ṣe bí ohun tí olódùmarè kò lọ́wọ́ sí, Alèwílèṣe, Aṣèkanmákù. Ìgbà mìíràn a tún lè sọ pé ọlọ́run nìkan ló gbọ́n, ó rí ohun gbogbo, ó sì lè ṣe ohun gbogbo, Arínúróde Olùmọ̀ràn ọkan, Yorùbá sọ pé “Amòòkùn ṣolè bí Ọba ayé kò ri, Ọba ọ̀run ń wò ó, èyí túmọ̀ sí wí pé kò sí ohun tí a ṣe ní ìkọ̀kọ̀ tí Olódùmarè kò rí, kedere ni lójú Olódùmarè, àwọn òrìṣà ló máa ń jẹ àwọn arúfin ní ìyà ṣùgbọ́n Olódùmarè ló máa ń dájọ́ fún wọn, fún àpẹẹrẹ ní ìgbà kan gbogbo òrìṣa fẹ̀sùn kan ọ̀rúnmìlà níwájú olódùmarè lẹ́yin tí tọ̀tún tòsì wọ́n rojọ́ olódùmarè dá ọ̀rúnmìlà láre, odù ifá kan jẹri sí eléyìí, odù náà lọ báyìí “Ọ̀káńjùa kì í jẹ́ ka mọ nǹkan pínpín, Adíá fun odù. Mẹ́rìndín lógún níjọ́ ti wọn ń jìjà àgbà relé olódùmarè, nígbà tí àwọn ọmọ ìrúnmọlẹ̀ mẹ́rẹ̀ẹ̀rìndínlógún tán ń jìjà ta ni ẹ̀gbọ́n ta ni àbúrò láàárin ara wọn, wọ́n kẹ́jọ́ lọ sódọ̀ olódùmarè, níkẹyìn, olódùmarè dá ẹjọ́ pé èjìogbè ni àgbà fún àwọn odù yókù. Yorùbá gbàgbọ pé onídàjọ́ òdodo ni olódumarè, ìdí nìyí tí Yorùbá fi ń sọ pé ọlọ́run mú u tàbí ó wà lábẹ́ pàṣán ‘Olódùmarè. Òyígíyigì ọba Ọta àìkú fẹ̀rẹ̀kufẹ̀, a kì í gbọ́kú Olódùmarè. Tí a bá tún wo Ọ̀kànrànsá (odù ìfa) òun náà tún sọ pe olódùmarè kì í ku, fún àpẹẹrẹ, Odù ọ̀kànrànsá yìí sọ pé:
Ọ̀dọ́mọdé kì í gbọ́kú asọ
yẹyẹyẹ laṣọ ogbó
Olódùmarè náà ni Ọba àìrí, àwámárìdí Yorùbá tún gbà pé ó jẹ Ọba mímọ́ tí kò léèérí, alálà funfun òkè. Ìgbàgbọ́ Yorùbá ni pé bí àwọn áńgẹ́lì tí jẹ́ Olùrànláwọ́ fún Olódùmarè lóde ọ̀run ni àwọn òrìṣà náà jẹ́ aṣojú rẹ̀ lóde ìṣálayé, àwọn òrìṣà wọ̀nyí jẹ́ alágbàwí àwọn ènìyàn níwájú olódùmarè. A gbọ́ wí pé ìbáṣepọ̀ wà láàárin àwọn òrìṣà tàbí òòṣà ilẹ̀ Yorùbá àti Olódùmarè, àwọn Yorùbá gbàgbọ́ pe òòṣà wọ̀nyí nì wọ́n lè rán sí olódùmarè yálà láti tọrọ nǹkankan lọ́wọ́ rẹ̀ tàbí dúpẹ́ lọ́wọ́ rẹ̀ fún ohun ribiribi tí ó ṣe fún wọn. Erò yìí hàn nínú òwe Yorùbá kan pé “ẹni mojú ọwá là ń bẹ̀ sọ́wá, olójú ọwá kan kò sí bíkòṣe ayaba”. Ìdí nìyí tí ó fi jẹ pé bí a bá fẹ́ kí Ọba ṣe ohun kan fún ni a ó bẹ ayaba sí i, ipò alágbàwí láàárin àwọn abòòṣà àti olódùmarè ni àwọn òòṣà wà.
Ponun Erékùṣù Man
je owonina ni orile-ede ni Europe.
Àsìá ilẹ̀ Àrúbà
je asia orile-ede Aruba
Àsìá ilẹ̀ Erékùṣù Ascension
Àsìá ilẹ̀
Agbègbè Ìjọba Ìbílẹ̀ Port Harcourt
thumb|Agbègbè ìjọba Ìbílẹ̀, Port Harcourt. Agbegbe Ijoba Ibile Port Harcourt je ijoba ibile ni Ipinle Rivers ni Naijiria. Ibujoko re wa ni Port Harcourt
Lẹ́yìn ọdún mẹ́ta
Leyin odun meta
Lẹ́yìn ọdún mẹ́ta
Ohun t’ó bá gba ni lọ́jọ́ ogun
Òun l’ó yẹ ká wárí fún bíi gbanigbani
Ohun t’ó bá gba ni sìlẹ̀ lọ́jọ̀ ọ̀ràn
Òun ló yẹ ká sátọ̀ bíi olùgbèjà
Ṣéb’Olùfọ̀n ni kò jógun ó jà l’Ẹ́rìn
Ṣeb’Ájàlá Ṣàngó ni kò jógun ó kó Kòso
Àní ‘hun t’ó bá gba ni làá sin
Ṣùgbọ́n Òbìrí ayé ti yí bìrí
Ponun Gibraltar
thumb|Pọ́nún-ùn Gibraltar. je owonina ni orile-ede ni Europe.
Ojúewé Àkọ́kọ́
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Júpítérì
Awon astronomer ayeijoun mo Júpítérì, be sini o je gbigbo ninu esin ati asa awon eniyan igba na. Awon ara Romu soloruko fun osa Romu to unje Júpítérì. Ni wiwo lati Aye, Júpítérì le de itobi ihan −2.94, eyi so di ohun tomolejulo keta ni ojusanmo ale leyin Osupa ati Aguala. (Marsi le mole bi Júpítérì fun igba soki ni awon ojuami pato kan ni ojuiyipo re.)
Kim Clijsters
Kim Antonie Lode Clijsters (ojoibi 8 June 1983) je alagbata boolu tenis omo orile-ede Belgium.
Ojúewé Àkọ́kọ́
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Júpítérì
Júpítérì lati bere je haidrojin pelu ikan-ninu-idamerin isupo to je helium; o si tun se e se ko ni inu alapata awon apilese wiwuwo. Nitoripe o un yipo kiakia, iwoiri Júpítérì je bi obiriki afelegbe (o wu die sita ni agedemeji re). Ojuorun ode re je yiyasoto si orisirisi egbe ni ila-idubule otooto, to un fa iji ati rudurudu legbe awon bode to unkanra won. Esi eyi ni Great Red Spot, iji omiran kan to ti je mimo lati orundun 17k nigbati o koko je riri pelu teleskopu. To yika planeti yi ni sistemu oruka planeti ati ayikagberigberin alagbara. Be si tun ni o ni awon osupa 63, ninu won ni awon osupa gbangba merin ti won unje awon osupa Galilie ti won koko je wiwari latowo Galileo Galilei ni 1610. Ganymede, eyi totobijulo ninu awon osupa yi ni diamita totobiju planet Mercury lo.
Júpítérì ti je wiwakiri ninu lopolopo igba pelu oko-ofurufu roboti, agaga nigba awon iranlose ifokoja Pioneer ati Voyager ati leyin won pelu Galileo orbiter. Oko iwadi to pese lo si Júpítérì ni oko-ofurufu to unlo si Pluto, New Horizons ni opin February 2007. Oko iwadi yi lo iwolura lati odo Júpítérì lati fun ni isare pupo. Awon iwakiri ojowaju ninu sistemu Jofia ni wiwa omi ti tinyin bo mole ninu osupa Europa.
Ìdiramú
Júpítérì je kiki elo elefuufu ati olomi. Ohun ni o tobijulo larin awon omiran efuufu mererin ati bakanna planeti totobijulo ninu sistemu orun pelu diamita 142,984 km ni agedemeji re. Ikisi Júpítérì, 1.326 g/cm³, ni ekeji to gajulo larin awon planeti omiran efuufu. Sugbon, ikisi re kereju ti awon planeti onile mererin lo.
Ìkósínú
Oke ojuorun Júpítérì je bii 88–92% haidrojin ati 8–12% helium gegebi inuogorun itobi tabi ida awon igbonwo efuufu (see table to the right). Nitoripe atomu helium kan ni bi isupo lona merin ti atomu hydrogen kan, ajoropo yato nigbati a ba wo bi ipin isupo ti atomu kookan mu wa. Nitorie ojuorun je bi 75% haidrojin ati 24% helium gegebi isupo, pelu bi ikan ninuogorun yioku isupo je awon apilese yioku. Inu re loun ni awon eroja kiki bi be to je pe ipin je 71% hydrogen, 24% helium ati 5% awon apilese yioku bi isupo. Ojuorun re ni iye tasere metani, oru omi, ammonia, ati awon adapo ti won ni silicon. Bakanna awon iye tasere carbon, ethane, haidrojin onisulfur, neon, oxygen, phosphine, ati sulfur. Ipele to bo sode julo ojuorun re ni awon crystal ammonia gigan. Through infrared and ultraviolet measurements, trace amounts of benzene and other hydrocarbons have also been found.
Nipile lori iwo ipele awo, Satu je lilero pe o je bakanna ni ajokopo mo Júpítérì, sugbon awon efuufu omiran Uranu ati Neptu ni haidrojin ati helium didinku lafiwe. Sugbon, nitori ailewole awon oko iwadi si ojuorun awon planeti ti won jinna ju Júpítérì lo, ko si awon nomba pato to daju fun ijantirere awon apilese towuwoju fun awon planeti wonyi.
Àkójọ
thumb|left|Approximate size comparison of Earth and Jupiter, including the Great Red Spot Júpítérì je lona 2.5 isupo apapo gbogbo awon planeti yioku ninu Sistemu Orun—eyi supo to be to fi je pe arin iwuwo re pelu Orun wa loke ojude Orun ni 1.068 itande orun lati inu arin Orun. Botilejepe planeti yi tobi ju Aye lo pelu diamita lona 11 ti Aye, kikisi re din ju ti Aye lo daada. Itobinu Júpítérì je adogba mo 1,321 ti Aye, sibesibe planeti na supo lona 318 lasan ju Aye lo. Jupiter has a radius equal to 0.10 times the radius of the Sun, and has a mass of 0.001 times the mass of the Sun, making them approximately equal in density. Eyo iwon "isupo Júpítérì" kan (MJ or MJup ) lo unsaba je lilo lati juwe isupo awon ohun miran, agaga awon planeti odeorun ati awon brown dwarfs. Bi be, fun apere, planet odeorun HD 209458 b ni isupo 0.69 M J, nigbati COROT-7b ni isupo 0.015 M J.
Awon afijuwe elero fihan pe to ba je pe Júpítérì ni iye isupo to poju iye to ni bayi lo, planeti na yio funpomora. Nitoripe fun iyato die ni isupo, itande ko ni fi be yato, ati pe ni bi isupo Júpítérì merin soke inu re yio je jijofunpo gidigidi labe agbara irelura ti yio posi to fi je pe itobinu planeti na yio "dinku" botilejepe iye elo ti po si. Nitorie, Jupiter je lilero pe o ni diamita totobi fun iru ajokopo planeti na ati ti itan iyojade le se. Imuse ifunpo siwaju pelu iposi isupo yio tesiwaju titi ti igbanaje irawo to se e ri yio fi sele bo se wa ninu awon brown dwarf onisupo niunla pelu isupo Júpítérì 50. eyi lo fa ti awon atorawo kan se unpe ni "irawo akuna" (failed star), botilejepe ko daju boya awon ona imuse to unfa ida awon planeti bi Júpítérì je ikanna bi ti awon ona imuse ida opolopo awon sistemu irawo.
Botilejepe Júpítérì yio fe lati je lona 75 isupo yi ko to le sedadipo haidrojin lati di irawo, arara pupa kikerejulo je bi 30 ninuogorun lasan ni titobijulo itande ju Júpítérì lo. Sibesibe, Júpítérì si un setanjade oru/igbona ju iye to ungba latodo Orun lo. Iye oru to un wa lati inu planeti na fe tto dogba mo apapo itanjade orun to un gba. Itanjade oru yioku yi un wa pelu iseise Kevin-Hemholtz nipa irunpo alailekoja. Ona imuse yi unfa ki planeti na o funpo bi 2 cm lodoodun. Nigba to koko je dida, Júpítérì gbona ju bayi lo, o si ni diamita to po lona meji ju bayi lo.
Ìdiramú inú
right|thumb|This cut-away illustrates a model of the interior of Jupiter, with a rocky core overlaid by a deep layer of [[metallic hydrogen.]] Júpítérì je lilero pe o ni inu kiki pelu adalu awon apilese, ipele ayipoka liquid haidrojin onide olomi pelu helium melo kan, ati ipele ode to kun fun haidrojin igbonwo. Leyin outline die yi, iyoku ko daju. Inu re unsaba je jijuwe bi alapata, sugbon ekunrere akojopo re je aimo, be na lo ri fun awon ini eroja to wa ni awon igbonasi ati itemo awon ibu/ijin na (e wo isale). Ni 1997, iwon irelura lo fi dalaba pe o ni inu, lati safihan isupo lona lati 12 de 45 ti isupo Aye tabi bi 3%–15% gbogbo isupo Júpítérì. Pe inuarin wa nigba kan ninu itan Júpítérì je didalaba pelu awon afijuwe iseda planeti to so pe inuarin alapata tan yinyin koko wa to supo to be to lati kojo opo haidrojin ati helium re latodo nebula orunakoko. Ti a ba gba pe o wa, o le ti funpo bi iwo igbona sita haidrojin onide olomi gbigbona ba se un dalu mo inuarin yiyo to si gbe awon akoonu re lo si ibi giga ninu planeti na. Inuarin le mo si rara bayi nitoripe awon iwon irelura ko daju to lati fihan pe ko je be rararara.
Aidaju afijuwe na je nitori iye ipoto asise ninu awon paramita wiwon: ikan ninu awon afisodipupo alayirapo (J6) to je lilo lati fi juwe igba irelura planeti na, atanka alagedemeji Júpítérì, ati igbonasi re ni itemo 1 bar. Ireti ni pe iranlose JUNO, ti yio gbera ni 2011, yio se idikun awon asise awon paramita wonyi, lati mulosiwaju wa si isoro inuarin.
Agbegbe inuarin je yiyika pelu haidrojin onide kiki, to fe sode de bi 78 ninuogorun atanka planeti na. Helium kikan bi ojo ati neon unro sile latinu ipele yi, lati mu idinku ijantirere awon apilese wonyi wa ninu oke ojuorun.
Loke ipele haidrojin onide na ni ayika inu alaridenuwo ti haidrojin. Ninu ijin yi, igbonasi po ju igbonasi elewu lo, fun haidrojin to je 33 K lasan (e wo haidrojin).Ni ipo yi, ko si iyato isaye olomi ati elefuufu - haidrojin je sisope o wa ni ipo asan supercritical. Sibesibe, o rorun lati wo haidrojin bi efuufu ni ipele oke to unfe si sale lati isu ipele de ijin to to 1,000 km, ati bi olomi ni awon ipele jijinju. Logidi, ko si bode kedere kankan - efuufu di gbigbona ati kiki bo se unwale felefele.
Igbonasi ati itemo ninu Júpítérì unposi titi de inuarin. Ni agbegbe phase transition nibi ti haidrojin-to je gbigbegbona koja ojuami ewu—di onide, o je gbigbagbo pe igbonasi je 10,000 K be e sini itemo je 200 GPa. Igbonasi ni bode inuarin je jijeye pe o je 36,000 K beesini itemo inu je bi 3,000–4,500 GPa.
Afẹ́fẹ́àyíká
Júpítérì lo ni afefeayika planeti totobijulo ninu Sistemu Orun, o gun to 5000 km. Nitoripe Júpítérì ko ni ojude, ipile afefeayika re je gbigba bi ojuami ibi ti itemo afefeayika ti dogba mo 10 bars, tabi ona mewa itemo lori Aye.
Awon ipele isujo
Ipele isujo je bi 50 km ni jijin lasan, be sini o ni o ni iruipele meji: iruipele kiki labe ati agbegbe tinrin hihan die. O si tun se e se ki ipele tinrin isujoomi kan o wa labe ipele ammonia, bo se han pelu isana monamona ti won je gbigbamu ninu afefeojuorun Júpítérì. (Omi je igbonwo olopo kan to le gbe idira kan, bi be o le se iyato idira to ye lati se monamona.) Awon ijuwo idira onina yi le lagbara lona egberun ju monamona Aye lo. Awon isujo omi le da ijiara ti igbona lati inu ungbe kiri.
Awo osan ati brown inu isujo Júpítérì wa lati iwusoke awon adapo ti won unyi awo won pada nigbati won ba dojuko imole ultraviolet lati odo Orun. ohun to wa ninu awon adapo wonyi ko daju, botilejepe fosforu, sulfur tabi boya haidrokarbon ni won je gbigbagbo pe won je. Awon adapo alawo yi, ti won unje kromofori, undalu po mo awon isujo liloworo iruipele isale. Awon ibiamure je dida nigbati awon ahamo igbonalatinu ti won unbu soke ba da ammonia crystallizing ti won bo awon isujo isale wonyi.
Iteju ipo rirele Júpítérì tumosi pe awon oriopo ungba itankale orun didin nigbogbo igba ju agbegbe alagedemeji planeti na lo. Sugbon igbonalatinu ninu planeti na ungbe okun pupo lo si awon oriopo, eyi un unmu idogba ba awon igbonasi ti won wa ni ipele isujo.
Edward Mills Purcell
je onimosayensi to gba Ebun Nobel ninu Fisiksi.
Júpítérì
Oju Pupa Ninla ati awon vortices miran
thumbnail|250px|This dramatic view of Jupiter's Great Red Spot and its surroundings was obtained by [[Voyager 1 on February 25, 1979, when the spacecraft was 9.2 million km (5.7 million mi) from Jupiter. Cloud details as small as 160 km (100 mi) across can be seen here. The colorful, wavy cloud pattern to the left of the Red Spot is a region of extraordinarily complex and variable wave motion. To give a sense of Jupiter's scale, the white oval storm directly below the Great Red Spot is approximately the same diameter as Earth.]]
Lẹ́yìn ọdún mẹ́ta
Lẹ́yìn ọdún mẹ́ta
Ọmọ adáríhunrun ò níran olóore ...
Agbègbè Ìjọba Ìbílẹ̀ Potiskum
wa ni Naijiria
Lẹ́yìn ọdún mẹ́ta
Lẹ́yìn ọdún mẹ́ta
Asiri alabosi
Àṣírí alábòsí
Bí abẹ́rẹ́ bí abẹ́rẹ́ là ń ṣèké
B’írọ́ bá fẹ́ k’ó máa báfẹ́fẹ́ siré
Òtìítọ́ ò ní gbé ‘ṣè t’ó sì dunra
Júpítérì
Oju Pupa Ninla ati awon vortices miran
Ini to gbajumojulo ti Júpítérì ni ni Oju Pupa Ninla, iji olodi-ijiyipo to unsele nigbogbo igba to budo si 22° ariwa agedemeji to tobiju Aye lo. O ti je mimo pe o kere ju o wa lati 1831, o se e se ko je lati 1665. Awon afijuwe onimathimatiki da laba pe iji na je lekanlekan ati pe o se e se ko je ini planeti na to wa ni gbogbo igba. Iji yi tobi to be to fun awon telikopu ni Aye ti won ni aperture of 12 cm tabi titobijubelo le fi seewo.
Lẹ́yìn ọdún mẹ́ta
Àṣírí alábòsí
Òtíìtọ́ kò ní sáré jù ‘gbín
Kíprù
Kíprù tabi Orile-ede Olominira ile Kíprù je orile-ede erekusu ni Eurasia.
Júpítérì
Oju Pupa Ninla ati awon vortices miran
Iji yi to ri bi oval unyipo lonaodiago, pelu akoko bi ojo mefa. Awon The Great Red Spot's egbegbe Oju Pupa Ninla je 24–40,000 km × 12–14,000 km. O tobi to lati gba planeti meji tabi meta to ni diamita Aye. Ojuibigiga pipojulo iji yi je bi 8 km loke ayika awon ori isujo.
Lẹ́yìn ọdún mẹ́ta
Àṣírí alábòsí
Ibi t’írọ́ bá ṣubú sí l’òtíìtọ́ ó ti kì í mọ́lẹ̀
Júpítérì
Oju Pupa Ninla ati awon vortices miran
Awon iru iji bayi wopo ninu afefeojuorun onisoro awon efuufu omiran. Bakanna Júpítérì tun ni awon oval funfun ati brown ovals, ti won kere ti won ko ni oruko. Awon oval funfun ni isupo bibale lafiwe ni afefeojuorun oke. awon Brown ovals je liloworo won si wa ninu ipele isujo deede. Awon iru iji bayi le to fun wakati die tabi sele to opo odunrun.
Lẹ́yìn ọdún mẹ́ta
Àṣírí alábòsí
Ẹ má jẹ ń f’àkàwé gbàgbé alábòsí
Ẹ má jẹ ń sàròyé gbàgbé oníṣẹ́ ibi
Júpítérì
Oju Pupa Ninla ati awon vortices miran
Ko to di pe Voyager fihan pe ini na je iji, eri wa pe oju na ko se e sabase pelu ini jijin kankan lojude planeti na, nitoripe Oju na nyipo ni otooto lafiwe mo afefeojuorun yioku, nigba miran ni kiakia ati nigba miran ni diedie. Nigba itan akoole re o ti rinajo lopo igba yipo planeti na lafiwe si aseami ayipo gbaingbanin labe re yiowu to ba wa.
Lẹ́yìn ọdún mẹ́ta
Àṣírí alábòsí
Bàbá àlùsì tí mo fẹ sọ̀rọ̀ bá l’Obìnrin ti jàrábà
Júpítérì
Oju Pupa Ninla ati awon vortices miran
Ni 2000, ini afefeojuorun kan je dida nibi idajiojuorun apaariwa to jo Oju Pupa Ninla, sugbon to kerejulo. Eyi je dida nigbati awon iji bi oval funfun kekere darapo lati da ini kan soso—awon oval fufun kekere meta yi koko je siseakiyesi ni 1938. Oruko ini todarapo ni Oval BA, o si ni oruko alaje Oju Pupo Kekere. Latigbana o ti posi ni kikankikan o si ti yi awo re si pupa lati funfun.
1 July
30 June | 1 July | 2 July ---
Lẹ́yìn ọdún mẹ́ta
Àṣírí alábòsí
Wọn gba ṣòkòtò nídìí àgbààyà tán ...
Radiomu
Rédíọ́mù jẹ́ ìpilẹ̀ṣẹ̀ kẹ́míkà tó ní àmì-ìdímọ̀ Ra àti nọ́ḿbà átọ̀mù 88.
Lẹ́yìn ọdún mẹ́ta
Àṣírí alábòsí
Eyi fara, eyi foro
Èyí fàrà tọ̀hún fòró
Ìran ajá kan kìí mọ baba t’ó bá wáyé
Ẹjọ́ ajá kọ́, ohun a dá májá ni
Ìran òbúkọ kì í m’ọkọ iyá rẹ̀
Itú ò lẹ́ṣẹ̀ rárá, kádàrá ìran wọn ni
Ọmọ adáríhunrun tí kò lólú ni wọn ń pè ní t’àlè
Baba alábẹ́ oró t’idìí Obìnrin jẹ lógún
Aya aláya lo wò lásán loò gbádùn
Ọjọ ọ̀kẹ́rẹ́ ti ń fọ epo...
Ọ̀sọ́ òdì.
Ìran ajá kan kì í mọ baba t’ó bá wáyé
Ẹjọ́ ajá kọ́, ohun a dá májá ni
Àsìá ilẹ̀ Austrálíà
Àsìá ilẹ̀ Australia
Júpítérì
Awon oruka planeti
thumb|right|The [[rings of Jupiter.]]
Júpítérì ni sistemu faint oruka planeti die to ni igesoto meta: an inner toru awon inu particles ti won unje halo, oruka to mole lafiwe, ati oruka gossamer ode. Awon oruka yi da bi pe won je eruku, laije yinyin bi ti awon oruka Saturn. Oruka agba se e se ko je sise lati owo awon eroja to ta kuro lodo awon ajaeyin Adrastea ati Metis. Eroja to je pe yio bo pada sinu osupa na je fifa sinu Júpítérì nitori agbara irelura to ni. Ojuonaiyipo eroja te lo sodo Júpítérì be sini eroja tuntun unje fifikun pelu ifaragbara miran. Lona kanna ni awon osupa Thebe ati Amalthea da iru ohun inu meji ti oruka gossamer. Eri tu wa fun oruka alapata to sopo mo eti ojuonaiyipo Amalthea to se e se ko  je idoti ifaragbara osupa na.
Ìgbéringbérinàyíká
right|250px|thumb|[[Aurora (astronomy)|Aurora on Jupiter. Three bright dots are created by magnetic flux tubes that connect to the Jovian moons Io (on the left), Ganymede (on the bottom) and Europa (also on the bottom). In addition, the very bright almost circular region, called the main oval, and the fainter polar aurora can be seen.]] Jupiter's broad Papa igberin Júpítérì gbagada ni agbara lona 14 ju ti Aye lo, lati 4.2 gauss (0.42 mT) ni agedemeji de 10–14 gauss (1.0–1.4 mT) ni awon oriopo, eyi so di eyi tolagbara julo ninu Sistemu Orun (ayafi awon  ojuorun). Papa yi je gbigbagbo pe ounwa latodo awon iwo eddy—irelo lilo awon eroja conducting materials—larin inu haidrojin onide. Awon ileru ni osupa Io unfon iye gbangba sulfur oloksijinmeji lati da toru efuufu kan leti ojuonaiyipo osupa na. Efuufu na je sisodi ioni ninu igberinojuorun lati da awon ioni sulfur ati oxygen. Awon wonyi, lapapo mo awon ioni haidrojin to unwa latodo afefeojuorun Júpítérì, da form a plasma sheet ninu pete alagedemeji Júpítérì. Plasma na ninu sheet unjoyipo pelu planeti na lati fa ibajeida papa igberin oriopomeji si aboigberin (magnetodisk). Awon elektroni inu plasma sheet unfa ami radio alagbara toun fa ibu larin 0.6–30 MHz.
Lati bi 75 itanka Júpítérì lati odo planeti na, ibasepo igberinojuorun na mo iji orun unfa  bow shock. Eyi to yi igberinojuorun Júpítérì ka je a magnetopause, to budo si eti inu magnetosheath—agbegbe larin re ati bow shock. Iji orun unsebasepo mo awon agbegbe yi, lati fa igberinojuorun na ni lee side Júpítérì to si unfa sita titi to fi fe de ojuonaiyipo Saturn. Awon osupa Júpítérì merin titobijulo ni gbogbo won yipolojuona to wa ninu igberinojuorun Júpítérì, eyi unda ao bo won lowo iji orun.
Lẹ́yìn ọdún mẹ́ta
Ọ̀sọ́ òdì.
Ìran òbúkọ kì í m’ọkọ ìyá rẹ̀
Frits Zernike
je onimosayensi to gba Ebun Nobel ninu Fisiksi.
Lẹ́yìn ọdún mẹ́ta
Ọ̀sọ́ òdì.
Itú ò lẹ́ṣẹ̀ ràrá, kádàrá ìran wọn ni
Ọmọ adáríhunrun tí kò lólú ni wọn ń pè ní t’àlè
Baba alábẹ́ oró t’ídìí Obìnrin jẹ lógún
B’óo bá ti r’ábo l’abẹ́ẹ̀ rẹ ń dide
Aye aláya lo wò lásán loò gbádùn
Ọjọ ọ̀kẹ́rẹ́ ti ń fọ epo
Epo rẹ̀ ò kún ‘kòkò kan ṣoṣo
Ọjọ́ t’ólógbò ti ń gbówùú arúgbó...
Akẹ́kọ̀ọ́ t’ó ṣẹ̀ṣẹ̀ wọ Yunifásítì
Gbogbo ẹní ṣẹ̀ṣẹ̀ dé
Júpítérì
Ìgbéringbérinàyíká
Igberinojuorun Júpítérì lounfa itujade kikan radio lati awon agbegbe oriopo planeti na. Isele ileru inu osupa Jofia Io (e wo isale) untu efuufu sinu igberinojuorun Júpítérì, lati fa torus of particles kakiri planeti na. Bi Io se unrelo ninu toru yi, ibasepo na unfa iru Alfvén to ungbe elo to ti di ioni sinu awon agbegbe oriopo Júpítérì. Nipa bayit, awon iru radio unje fifa wa pelu cyclotron maser mechanism, okun re si unje gbigberinna (transmitted) sita legbe ojude to ri bi aro. Nigbati Aye ba rekoja aro yi awon itujade radio latodo Júpítérì le ju itujade radio orun lo.
Lẹ́yìn ọdún mẹ́ta
Akẹ́kọ̀ọ́ t’ó ṣẹ̀ṣẹ̀ wọ Yunifásítì
Ẹ kú oríire
Júpítérì
Ìgbàyípa ati iyirapo
Júpítérì nikan soso ni planeti to ni arin isupo pelu Orun to dubule si ode itobisinu Orun, botilejepe eyi je 7% lasa itanka Orun. Nomba-arin ijinna larin Júpítérì ati Orun je 778 million km (bi ona 5.2 nomba-arin ijinna lati Aye de Orun, tabi 5.2 AU) o si unpari ojuonaiyipo kan ni odun 11.86. Eyi je meji-ninu-idamarun akoko ojuonaiyipo Saturn, lati da 5:2 orbital resonance larin awon planeti meji titobijulo yi ninu Sistemu Orun. ojuonaiyipo awodie (elliptical orbit) Júpítérì je te ni 1.31° lafiwe mo Aye. Nitori eccentricity 0.048, ijinna lati Júpítérì ati Orun yato bi 75 million km larin perihelion ati aphelion, tabi ojuami ijinna tosunmojulo ati tojinnajulo planeti na leba ipase ojuonaiyipo ni titelentele.
Lẹ́yìn ọdún mẹ́ta
Akẹ́kọ̀ọ́ t’ó ṣẹ̀ṣẹ̀ wọ Yunifásítì
Ẹ kú àjàyè tẹ́ẹ mọ̀ ọ́n jà
J. M. G. Le Clézio
Jean-Marie Gustave Le Clézio (ojoibi 13 April 1940) je olukowe to gba Ebun Nobel ninu Litireso.
Lẹ́yìn ọdún mẹ́ta
Akẹ́kọ̀ọ́ t’ó ṣẹ̀ṣẹ̀ wọ Yunifásítì
Àlááfíà kọ́ lẹ wà bí?
Júpítérì
Ìgbàyípa ati iyirapo
Ojuite ipo Júpítérì kere lafiwe: 3.13° lasan. Nitorie planeti yi ko ni iyipada igba tosekoko, lodi si Aye ati Mars fun apere.
Lẹ́yìn ọdún mẹ́ta
Akẹ́kọ̀ọ́ t’ó ṣẹ̀ṣẹ̀ wọ Yunifásítì
Ará le tàbí kò le?
Ṣ’ẹ́ṣin ń joko koro koro
Júpítérì
Ìgbàyípa ati iyirapo
Iyirapo Júpítérì ni o yarajulo ninu gbogbo awon planeti inu Sistemu Orun, ounpari iyirapo kan lori ipo re larin wakati mewa odin die; eyi da iwu alagedemeji to se e fojuri pelu teliskopu lati Aye laisisoro. Iyirapo yi unfe centripetal acceleration ni alagedemeji bi 1.67 m/s², lafiwe mo irelura ojude alagedemeji 24.79 m/s²; bi be  net acceleration iseku to wa ni ojude alagedemeji je bi 23.12 m/s² lasan. Planeti na ri bi obiriki oblate, to tumosi pe diameter ni agedemeji re gunju diamita  larin  awon oriopo re lo. Lori Júpítérì, diamita alagedemeji je 9275 km nigigun ju diamita arin awon oriopo re lo.
Lẹ́yìn ọdún mẹ́ta
Akẹ́kọ̀ọ́ t’ó ṣẹ̀ṣẹ̀ wọ Yunifásítì
Ṣé bàbà rẹ̀ ò yéé mì làbà làbà?
Ede Yorùbá ti t’ámòójútó
Júpítérì
Ìgbàyípa ati iyirapo
Nitoripe Júpítérì ki i se agbarajo lilekoko, afefeojuorun oke re ni iyirapo olotooto. Iyirapo afefeojuorun oriopo Júpítérì je bi iseju 5 poju ti afefeojuorun alagedemeji; awon sistemu meta lounje lilo gege bi itokasi, agaga nigbati a ba unyaworan iwon irelo awon ini afefeojuorun. System I je lati awon ojuibigbooro 10° A de 10° G; akoko re ni eyi tokerejulo ti planeti, ni 9h 50m 30.0s. System II lati gbogbo awon ojuibigbooro ni ariwa ati guusu awon wonyi; akoko re je 9h 55m 40.6s. System III koko je titumo latowo awon atorawo radio, o si baramu mo iyirapo igberinojuorun planeti na; akoko re ni iyirapo onibise Júpítérì.
2 July
1 July | 2 July | 3 July
Lẹ́yìn ọdún mẹ́ta
Akẹ́kọ̀ọ́ t’ó ṣẹ̀ṣẹ̀ wọ Yunifásítì
Nítorí afárá ìjọ́sí ti yí padà
Afárá sì ti d’okinni ...
Ọ̀gágun Múrítàlá dẹni àgbégbè
Mo dé ‘gbó mọláró
Mo dé ‘gbó Màkẹfun
N ò róye Ọba Ẹlẹ́fun
Mo dé ‘gbó Màkosùn
Dọ̀dàani ni mo dé
Mo ní Múrítàlá ńkọ́
Ẹ jọ̀wọ̀, ẹ bá mi wọ́gàá àwa lọ
Ẹ bá ní wá Múrítàlá ọmọ Mọ̀nmọ́dù ...
Iwe ti a yewo
Ọlátunjí Ọ́pédọ̀tun (2000), Àròfọ̀ Eléwì-odò  Oníbonoje Press ISBN 978-145-069-X, oju-iwe 17-32.
Olatunji Opadotun
link title
Àsìá ilẹ̀ Austríà
Àsìá ilẹ̀ Austríà je ti orile-ede Austríà
Werner Forssmann
je onimo sayensi to gba Ebun Nobel fun Iwosan.
Agbègbè Ìjọba Ìbílẹ̀ Rafi
wa ni Naijiria
Max Born
je onimosayensi to gba Ebun Nobel ninu Fisiksi.
Agbègbè Ìjọba Ìbílẹ̀ Rabah
Agbegbe Ijoba Ibile Rabah je ijoba ibile ni Ipinle Sokoto ni Naijiria. Ibujoko re wa ni Rabah
André Frédéric Cournand
thumb|André Frédéric Cournand je onimo sayensi to gba Ebun Nobel fun Iwosan.
Ogun Abẹ́lé Àkọ́kọ́ ilẹ̀ Lìbéríà
Ogun Abẹ́lé Àkọ́kọ́ ilẹ̀ Lìbéríà je ijakadi abele to sele ni Liberia lati odun 1989 titi di 1997. Ijakadi na fiku pa eniyan to to 250,000 o si fa ikopa Economic Community of West African States (ECOWAS) ati United Nations. Ipinu ijnu ogun ko pe rara nitoripe ni odun 1999 Ogun Abele Ikeji ile Laiberia tun bere.
Walther Bothe
je onimosayensi to gba Ebun Nobel ninu Fisiksi.
3 July
2 July | 3 July | 4 July -
Herta Müller
je olukowe to gba Ebun Nobel ninu Litireso. thumb|380px
Alfred Hitchcock
Sir Alfred Joseph Hitchcock, KBE (13 August 1899 – 29 April 1980) je ara Geesi oludari filmu ati onigbowo filmu.
Ogun Abẹ́lé Gríìsì
Ogun Abẹ́lé Gríìsì (ο Eμφύλιος [Πόλεμος], "the Civil War") was fought from 1946 to 1949 between the Greek governmental army, backed by the United Kingdom and United States, and the Democratic Army of Greece (ΔΣΕ), the military branch of the Greek Communist Party (KKE), backed by Bulgaria, Yugoslavia and Albania.
Ìtàn ilẹ̀ Áfríkà
Ìtàn ilẹ̀ Áfríkà
Ilorin
Ilorin ni olu-ilu Ìpínlẹ̀ Kwara ní ìwọ̀ oòrùn Nàìjíríà. Gégé bi abayori ìkà ènìyàn odun 2006 ní Nàìjíríà, ìlú Ilorin ní olùgbé 777,667, èyí mú kí ó jẹ́ ìlú keje tí ó ní olùgbé jùlo ní Nàìjíríà.
Àsìá ilẹ̀ Azerbaijan
Àsìá ilẹ̀ Azerbaijan je asia orile-ede Azerbaijan.
STS-47
STS-47 was the 50th Space Shuttle mission of the program, as well as the second mission of Space Shuttle Endeavour. The mission mainly involved conducting experiments in life and material sciences.
Joseph Omotoye
je olorin ara Naijiria.
Agbègbè Ìjọba Ìbílẹ̀ Rano
wa ni Naijiria
Willis Lamb
Willis Eugene Lamb Jr. je onimosayensi to gba Ebun Nobel ninu Fisiksi.
Bohriomu
Bohriomu je ipilese elegbogi pelu ami-idamo Bh ati nomba atomu 107.
Apáàríwá Kíprù
Apaariwa Kipru tabi Ariwa Kipru (Kuzey Kıbrıs), to je mimo fun ibise bi orile-ede Olominira Turki ile Apaariwa Kipru (TRNC) (Kuzey Kıbrıs Türk Cumhuriyeti, KKTC), ni de facto orile-ede olominira to budo si ariwa Cyprus.
Bala Mande
je omo orile-ede Naijiria ati gomina Ipinle Nasarawa tele.
STS-52
thumb|Ẹgbẹ́ aṣàgbékalẹ̀ STS-52.
Abdullahi Ibrahim
Abdullahi Ibrahim je agbejoro, oloselu ati alamojuto ara Naijiria. Tele o je Alakoso Oro Idajo ile Naijiria.
Dickinson W. Richards
Dickinson Woodruff Richards, Jr. (October 30, 1895 – February 23, 1973) je onimo sayensi to gba Ebun Nobel fun Iwosan.
Fránsíọ̀m
Fránsíọ̀m tabi Francium, mimo tele bi eka-caesium ati actinium K, je apilese kemika to ni ami-idamo Fr ati nomba atomu 87. O ni ikan ninu awon odionina tokerejulo larin gbogbo awon apilese ti a mo, bakanna ohun ni apilese aladanida keji tosowonjulo (leyin astatine). Fransiom je onide to je radioalagbara giga to n jera si astatine, radium, ati radon. Gege bi onide alkali, o ni agbara elektroni kan.
Francium je wiwari latowo Marguerite Perey ni Fransi (nibi ti apilese yi ti ri oruko) ni 1939. Ohun ni apilese togbeyin ti o je wiwari ninu adanida, kanran jije sisopapo. Lode yara ise-idanwo, francium sowon gidigidi, iye ipase je wiwari ninu alumoni aladalu uranium ati thorium, nibi ti isotopu francium-223 ti n je didasile to si n je jijera bibaun. Iye to kere bi 20–30 g (ounce kan) lowa nigba yiowu kakiri inu igbele Aye; awon isotopu yioku je alasopapo yanyan. Iye titobijulo ti o je kikojo lai isotopu yiowu ni isupo bi awon atomu 10,000 (ti francium-210) ti won je didasaye gege bi efuufu tutugidi ni Stony Brook ni 1997.
Gàbọ̀n
Gàbọ̀n, lonibise bi Orile-ede Olominira ara Gabon (République Gabonaise) je orile-ede ni iwoorun gbongan Afrika to ni bode mo Guinea Alagedemeji ni ariwaiwoorun, Cameroon ni ariwa, ati mo Orile-ede Olominira ile Kongo to lopo ni ilaorun ati guusu. Ikun-omi Guinea, apa Okun Atlantiki si iwoorun. Ile re tobi to 270,000 km² o si ni alabugbe to to 1,500,000. Oluilu ati ilu totobijulo re ni Libreville.
Lati igba ilominira latowo Fransi ni August 17, 1960, awon aare meta loti joba ni Gabon. Ni arin ewadun 1990, Gabon bere sistemu egbe oloselu pupo ati isepo oloselu tuntun to fi aye gba igbese aladiboyan kedere to si satunse opo awon ise ijoba. Gabon ti je omo-egbe alaije tigba gbogbo ni Igbimo Abo UN fun igba 2010-2011.
Low Isupo alabugbe kekere lapapo mo opo awon ohun alumoni ati idawosi aladani okere ti so Gabon di ikan ninu awon orile-ede to jomitoro julo ni Afrika, pelu HDI to gajulo ati GDP ti enikookan togajulo keta (PPP) (leyin Equatorial Guinea ati Botswana) ni agbegbe yi.
Agbègbè Ìjọba Ìbílẹ̀ Àríwá Remo
Agbegbe Ijoba Ibile Ariwa Remo je ijoba ibile ni Ipinle Ogun to wa ni Naijiria.
STS-53
thumb|Ìdarí STS- 53.
Agbègbè Ìjọba Ìbílẹ̀ Rijau
wa ni Naijiria
Àsìá ilẹ̀ àwọn Bàhámà
Àsìá ilẹ̀ àwọn Bàhámà je ti orile-ede àwọn Bàhámà
Kroatíà
Kroatíà tabi Orílẹ̀-èdè Olómìnira ilẹ̀ Kroatíà je orile-ede ni Guusuilaoorun Europe.
Ìṣiṣẹ́òkòwò
Ìṣiṣẹ́òkòwò (Economics) je sayensi awujo to unmo nipa imuwaye, ipinkiri, ati iraja awon oja ati iwofa.
Ọ̀rọ̀ òkòwò un se alaye bi awon okowo se unsise ati bi awon osise olokowo se un wuwa si ara won. Ituyewo olokowo unje mimulo kakiri awujo, ninu isowo, inawo ati ijoba, sugbon bakanna ninu iwa odaran, eko, the ebi, ilera, ofin, iselu, esin, social institutions, war, ati sayensi.
Itokasi
Ekonomie Wirtschaftswissenschaft ምጣኔ ሀብት اقتصاد Economía ܡܡܘܢܐ Economía Nafasorosira অর্থনীতি Keng-chè-ha̍k Иҡтисад Эканоміка Эканоміка Ekonomija Armerzh Икономика (наука) Economia Экономика Ekonomiks Ekonomie Ekonomia Economeg Økonomi Wirtschaftswissenschaft Majandusteadus Οικονομικά Economics Economía Ekonomiko Economia Ekonomia fa:علم اقتصاد Búskapur Économie Ekonomy Economie Eacnamaíocht Tarmaynys Riaghladaireachd Economía Kîn-chi-ho̍k 경제학 Տնտեսագիտություն अर्थशास्त्र Gospodarstvo Ekonomiko Ekonomi Economia Economica Hagfræði Economia כלכלה Ékonomi ಅರ್ಥಶಾಸ್ತ್ರ ეკონომიკა Экономика Somo la Uchumi Ekonomi Aborî Ekonomiya ເສດຖະສາດ Oeconomia Ekonomika Economie Ekonomika Economie dinske Közgazdaságtan Економија Toe-karena സാമ്പത്തികശാസ്ത്രം अर्थशास्त्र Ekonomi Economie अर्थशास्त्र 経済学 Samfunnsøkonomi Samfunnsøkonomi Êcononmie nov:Ekonomike Economia Iqtisodiyot pnb:اکنامکس وټپوهنه សេដ្ឋកិច្ច Ekonomiks Ekonomia Economia kaa:Ekonomika Economie Musiku Экономика (наука) sah:Экономика Economics अर्थशास्त्रं Economia Economics stq:Wirtschaft Ekonomia Econumìa ආර්ථිකවේදය Economics Všeobecná ekonomická teória Ekonomija Dhaqaale Економија Privreda Kansantalous Nationalekonomi Ekonomiya பொருளியல் İqtisat ఆర్థిక శాస్త్రము เศรษฐศาสตร์ Иқтисодиёт İktisat Економіка معاشیات Economia Kinh tế học Konömav Majandustiidüs 計學 Ekonomiya Koom-koom עקאנאמיק 經濟 Akuonuomėka 经济学
Agbègbè Ìjọba Ìbílẹ̀ Àríwá Afikpo
Agbègbè Ìjọba Ìbílẹ̀ Àríwá Afikpo jẹ́ ìjọba ìbílẹ̀ ní Ìpínlẹ̀ Ebonyi ní orílẹ̀-èdè Nàìjíríà. Olú agbègbè náà wà ní Ehugbo, Afikpo. Àwọn ìlú pàtàkì níbẹ̀ ni [Unwana]], Itim, Ohaisu, Nkpoghoro, Ugwuegu/Amaizu, Ozizza, Amasiri, Ibii/Akpoha. Èdè ìbílẹ̀ Igbo tí ó ń jẹ́ 'Ehugbo ni wọ́n máa ń sọ. Ìlú yìí kún fún àwọn àṣà Igbo tó jinná tí ó sì múnádóko àti àwọn ọdún ìbílẹ̀ bí i "ọdún iṣu tuntun" tí wọ̀n máa ń ṣe ní ìparí oṣù kẹjọ.
Kazimierz Nowak
thumb|Kazimierz Nowak Kazimierzu Nowaki (lati Ọdún 1897 títí di Osu Òwàrà Ọjọ kétàlá Ọdún 1937 je ọmọ Ìuí Polandi ti Ọjẹ arińninajo Oníweroým ati aya woran ti a bi ni ilu Stiryi.
Lehin Ogun àgbáyé alakọkọ ogbe ni ilu Poznani lati ọdún 1931 títí di ọdún 1936 Orin, ogun kẹkẹ jake jado ilu Aláẁọ dúdú. Orin irinajo ti oto egberun lọ́na ogoji kilomita (40.000 km). Owun ni eni akọkọ ti okọkọ ṣẹ́iru nkan bayi.
O ti kọ iṣẹ yi si inu iwe ti a pe orukọ rẹ ni Rowerem i pieszo przez Czarny Ląd (Kẹkẹ ati ẹsẹ jake jado ilẹ aláẁọ dúdú). Oku si ilu Poznani.
Agbègbè Ìjọba Ìbílẹ̀ Ado-Odo/Ota
Agbègbè Ìjọba Ìbílẹ̀ Ado-Odo/Ota jẹ́ ọ̀kan lára àwọn ìjọba ìbílẹ̀ tó wà ní Ìpínlẹ̀ Ògùn. Ọjọ́ kọkàndínlógún oṣù karùn-ún, ọdún 1989 ni wọ́n da sílẹ̀. Ìjọba ìbílẹ̀ yìí ni èyí tó tóbi ṣìkejì ní ìpínlẹ̀ Ogun. Olú-ìlú rè wà ní Ota 6.68333°N, 3.68333°W. Àwọn ìlú mìíràn ní agbègbè náà ni: Araromi-Alade, Ado-Odo, Agbara, Igbesa, Iju-Ota, Itele, Kooko Ebiye Town, Owode, Sango Ota àti bẹ́ẹ̀ bẹ́ẹ̀ lọ.
Ó ní ìwọ̀ ilẹ̀ tó tóbí tó 878 km2 àti èrò ènìyàn tó tó bíi 526,565 lásìkò ìkarí ti ọdún 2006. Ó jẹ́ ilẹ̀ tó dáa fún iṣẹ́ àgbẹ̀, wọ́n sì máa ń gbin ohun ọ̀gbìn bíi: Kòkó, Obi, Epo, kọfí, Ẹ̀gẹ́, Igi Ose, Àgbàdo, àti ẹ̀fọ́.
Àwọn Àwórì ló pọ̀ jù ní agbègbè yìí. Àmọ́, a ní àwọn ẹ̀yà mìíràn bíi Àwọn Ẹ̀gbá, Eguns, àti Yewas (Egbados). Lọ́wọ́lọ́wọ́, àwọn aàfin ọba mọ́kànlá ló wà ní ìjọba ìbílẹ̀ náà, tí ń ṣe: Olofin of Ado-Odo, Olota of Ota, Onilogbo of Ilogbo, Oloja Ekun of Igbesa, Onikooko of Kooko Ebiye, Onitele of Itele, Amiro of Ilamiro, Onitekun of Itekun, Olodan of Odan Abuja Sule, Alagbara of Agbara, Onigun of Odan-Abuja, Onikogbo of Ikogbo, Olu of Owode Ota, Olu of Atan Ota, Olu of Ijoko Ota àti Olu of Tigbo Ilu.
Kóòdù ìfìwéránṣe ti agbègbè náà ni 112.
Alága ìbílẹ̀ náà ni Hon. Sheriff Adewale Musa.
Ìjọba ìbílẹ̀ yìí ni Ààrẹ orílẹ̀-èdè Nàìjíríà tẹ́lẹ̀ rí, tí ń ṣe Olusegun Obasanjo ti wá, ibẹ̀ sì ni oko rẹ̀ wà, tó pè ní Obasanjo Farms.
Àsìá ilẹ̀ Báháráìnì
Àsìá ilẹ̀ Bahrain
Polykarp Kusch
je onimosayensi to gba Ebun Nobel ninu Fisiksi.
Agbègbè Ìjọba Ìbílẹ̀ Gúúsù Afikpo
Agbegbe Ijoba Ibile Guusu Afikpo je ijoba ibile ni Ipinle Ebonyi ni Nigeria. Ibujoko re wa ni Nguzu-Edda.
Agbègbè Ìjọba Ìbílẹ̀ Rimi
wa ni Naijiria
Abdullahi Adamu
Abdullahi Adamu je omo orile-ede Naijiria ati gomina Ipinle Nasarawa tele. Ni Oṣu Kẹta ọdun 2022, Abdullahi Adamu jẹ aarẹ ẹgbẹ Congress of Progressives, ẹgbẹ to poju ni Naijiria. In March 2022, Abdullahi Adamu was appointed president of the Congress of Progressives party, the majority party in Nigeria.
Daniel Bovet
Daniel Bovet (23 March 1907 – 8 April 1992) je onimo sayensi to gba Ebun Nobel fun Iwosan.
Àwọn ará Ilẹ̀gẹ̀ẹ́sì
Awon ara Ilegeesi je eya eniyan ati orile-ede eniyan ni Ilegeesi. Ede won ni ede Geesi.
Pẹ̀lẹ́
Pele
Pẹ̀lẹ́
Mo kí ìyáálé ilé kan pẹ̀lú ọ̀wọ̀ níjọ́sí,
Mo ní ‘Ẹ pẹ̀lẹ́, mà~’
Ó bá bínú, ó ní, ‘Mo jẹ́gbẹ́ ẹ kọ́ bùọ̀dá,
Tó fi ń ṣe mí ní. “Ẹ pẹ̀lẹ́ mà.”
Ó ṣe mí ní kàyééfi mo bẹ̀bẹ̀ gán-ín.
Mo ní, ‘Ẹ jọ̀wọ́, ẹ má mà bínú,
Èyí wá mú mi rántí ọ̀rọ̀ àwọn àgbà, ...
Irahun aja kan
Aja
Irahun
Ìráhùn Àjá Kan
Ìgbà tí mo kọ́kọ́ fojú bale ayé,
Mo gbà, ẹ ẹ̀ pọ́n mi lójú kankan.
Ẹ̀ ń kẹ́ mi, ẹ̀ ń gẹ̀ mí.
Ẹ ẹ̀ sì ṣàìfúnmi lóúnjẹ.
Àgàgà tẹ́ ẹ tún rámì akọ nísàlẹ̀,
Agbègbè Ìjọba Ìbílẹ̀ Rimin Gado
wa ni Naijiria
Pẹ̀lẹ́
Ìráhùn Àjá Kan
Bí i ká jẹ̀kọ ìdájí ni.
Níjọ́ eegun ẹran lásán,
Níjọ́ apẹ híha jẹ. ...