User:YuRi YuZi
World A-
Fortress
World A-
Tower
World A-
Fortress
World A-
Airship
World A-
Jet
World A-
Bowser's Castle
World A-
Ship
World A-
Tank
World A-
Hand Trap
World A-
Desert
World A-
Pyramid
Yajirobe in Russian: Ядзиробэ, Ядзиробе, Яджиробэ, Яджиробе
The list of Super Mario Odyssey kingdoms found/mentioned in Wikipedia
The list of Super Mario Odyssey gameplay pictures showing kingdoms found in Wikipedia
Super Mario Odyssey's Wikipedia page
Mario's Wikipedia page
Mushroom Kingdom's Wikipedia page
The list of Super Mario Odyssey's mentioned kingdoms in Wikipedia
Super Mario Odyssey's Wikipedia page
Empire State Building in popular culture
Moon
Minus World be like:
- "Floating" Princess Peaches
- "Dead" Bowsers
- Glitchy worlds
BONUS
The Filipino "AhBahKahDah" transcripted into Cyrillic (see https://www.youtube.com/watch?v=N63WjFWHCvU)
- Тайо на ат маг-арал
- Нг атинг А-БА-КА-ДА
- А БА КА ДА Э ГА ХА
- И ЛА МА НА НГА О ПА
- РА СА ТА У ВА Я
- Анг атинг А-БА-КА-ДА
- Кунг итоы алам нийо на
- Тайо на ат куманта
USSR anthem in English
I An unbreakable union of free republics, Great Russia has sealed forever. Long live, the creation by the people's will, The united, mighty Soviet Union!
Chorus I: Be glorified, our free Fatherland, Reliable stronghold of the people's friendship! Banner of the Soviets, banner of the people, May it lead from victory to victory!
II Through storms the sun of freedom shined on us, And Great Lenin illuminated our path. Stalin taught us to be faithful to the people, To labor and achievements we were inspired!
Chorus II: Be glorified, our free Fatherland, Reliable stronghold of the people's happiness! Banner of the Soviets, banner of the people, May it lead from victory to victory!
III We raised our Army in battles, And swept the vile invaders from the path! In battles we determine the fate of generations, We bring glory to our Fatherland!
Chorus III: Be glorified, our free Fatherland, Reliable stronghold of the people's glory! Banner of the Soviets, banner of the people, May it lead from victory to victory!
Japanese version of Play Nintendo terms in Romaji and Cyrillic
Romaji
Bācharu Konsōru de ninki shirīzu no rekishi o tadorou! Muryō de daunrōdo dekiru gēmu tte dōshitara asoberu no? Nintendō 3DS no tatchisukurīn wa dōshite tatchi suru to han'nō suru no!? HOME menyū o jōzu ni kasutamaizu suru ni wa? AR kādo kara kyarakutā ga tobidasu no wa dōshite? Itsuka wa gēmu o tsukuru shigoto ga shitai! Gēmu tte dō yatte tsukurareteiruno? Shimatta! Sofuto o wasurete kita!
Mario fukuwarai de asobou! Kurisumasu ni o uchi de kazaru minitsurī o tsukuttemiyō! Min'na shitteru!? Sūpā Mario-kun Harō~in wa fotopuroppusu de dai henshin! "Pēpā Mario Karā Supurasshu" no nuri e o purezento! Mario tanzaku o tsukutte miyou! Sutaffu jikiden!! Mario no irasuto ga dekiru made [Sūpā Mario shirīzu vol. 3] Nintendōkizzusupēsu kara nuri e purezento! [Sūpā Mario shirīzu vol. 2] Nintendōkizzusupēsu kara nuri e purezento! "Sūpā Mario Mēkā (Wii U)" Mario no orijinarukabegami o tsukurou! Dai kōkai! Mario kyaraben no tsukurikata Mario & Ruīji Ārupījī Pēpā Mario MIX ni tōjō suru dodekakurafuto o tsukutte miyou! Gēmude wa kon'na kanji! Happy Halloween! Mario to Ruīji ni hensō shi chaou! Nuri e purezento [Sūpā Mario shirīzu vol. 1]
Sūpā Mario Mēkā Kōsu Sakusei Kōza Mashiko to Yamamura Toshinose-hen Tenohira saizu no Famicom tōjō! Naizō sofuto o dai kōkai (1990 ~ 1993) Tenohira saizu no Famicom tōjō! Kinoko Ōkoku no kakureta sutā!? Kinopio dai tokushū Tenohira saizu no Famicom tōjō! Naizō sofuto o dai kōkai (1983 ~ 1986) Nintendō no gēmu tte Nihon to kaigai de doko ga chigau no!? Hana-kun & Fuda-sensei no hanafuda batoru dōjō!! "Koi-Koi" o asonde miyou Kono natsu, Rio de atsukunare! Hana-kun & Fuda-sensei no hanafuda batoru dōjō!! Hanafuda tte nani? Sūpā Mario Mēkā Kōsu Sakusei Kōza Mashiko to Yamamura Bangai-hen sono 2 Sūpā Mario Mēkā Kōsu Sakusei Kōza Mashiko to Yamamura Bangai-hen sono 1 Rio no shuyaku ni odoridero! Chū o mai, kyodai ni naru. Nan demo ari no tenisu batoru! Sūpā Mario Mēkā Kōsu Sakusei Kōza Mashiko to Yamamura Saishū-banashi Sūpā Mario Mēkā Kōsu Sakusei Kōza Mashiko to Yamamura Dai roku wa "Fainaru Fantajī VII" kara kura udo sansen!! Sūpā Mario Mēkā Kōsu Sakusei Kōza Mashiko to Yamamura Dai go wa "Choi teku" Subete wa koko kara umareru cho! [Vol. 7] Sūpā Mario Mēkā Kōsu Sakusei Kōza Mashiko to Yamamura Dai yon wa Sūpā Mario Mēkā Kōsu Sakusei Kōza Mashiko to Yamamura Dai san wa Sūpā Mario Mēkā Kōsu Sakusei Kōza Mashiko to Yamamura Dai ni wa Sūpā Mario Mēkā Kōsu Sakusei Kōza Mashiko to Yamamura Dai ichi wa "Choi teku" Kotoshi wa, Sūpā Mario 30 shūnen no toshida cho! [Vol. 6] Choite-kun ga gēmu shoppu ni yattekita [Vol. 5] "Choi teku" Mememememe sore, megateku~! [Vol. 4] Are? Choite-kun ga, “nendo” ni nacchatta!! [Vol. 2] Dōmo. Kono ba o o karishi te choi teku o hajime te mimashita. [Vol. 1]
Daigassō! Bando Burazāzu P: Manga Bābara-chan P Bābara & Ashurī Manga Bābara-chan P Bābara to Yamamura Kaihatsu sutaffu ga egaku! Supesharu komikku Ashurī no Harowin naito Susume! Kinopio Taichō Dai 10 kai: Aratanaru bōken Susume! Kinopio Taichō Dai 9 kai: Happī endo? Susume! Kinopio Taichō Dai 8 kai: Purezento Susume! Kinopio Taichō Dai 7 kai: Kinopio Taichō kyūshutsu sakusen Susume! Kinopio Taichō Dai 6 kai: Torokko Maunten nite Susume! Kinopio Taichō Dai 5 kai: Wingo to taiketsu Susume! Kinopio Taichō Dai 4 kai: Heihō no Machikado nite Susume! Kinopio Taichō Dai 3 kai: Sutāto no hanashi Susume! Kinopio Taichō Dai 2 kai: Kōgen no Kinoko Iwa nite Susume! Kinopio Taichō Dai 1 kai: Kyoro-hei no Rōru Shinden nite
Cyrillic
БАЧАРУ КОНСОРУ ДЭ НИНКИ ШИРИЗУ НО РЭКИШИ О ТАДОРОУ! МУРЁ ДЭ ДАУНРОДО ДЭКИРУ ГЭМУ ТТЭ ДОШИТАРА АСОБЭРУ НО? НИНТЭНДО 3ДС НО ТАТЧИСУКУРИН ВА ДОШИТЭ ТАТЧИ СУРУ ТО ХАН'НО СУРУ НО!? ХОМЭ МЭНЮ О ДЖОЗУ НИ КАСУТАМАИЗУ СУРУ НИ ВА? АР КАДО КАРА КЯРАКУТА ГА ТОБИДАСУ НО ВА ДОШИТЭ? ИЦУКА ВА ГЭМУ О ЦУКУРУ ШИГОТО ГА ШИТАИ! ГЭМУ ТТЭ ДО ЯТТЭ ЦУКУРАРЭТЭИРУНО? ШИМАТТА! СОФУТО О ВАСУРЭТЭ КИТА!
МАРИО ФУКУВАРАИ ДЭ АСОБОУ! КУРИСУМАСУ НИ О УЧИ ДЭ КАЗАРУ МИНИЦУРИ О ЦУКУТТЭМИЁ! МИН'НА ШИТТЭРУ!? СУПА МАРИО-КУН ХАРО~ИН ВА ФОТОПУРОППУСУ ДЭ ДАИ ХЭНШИН! "ПЭПА МАРИО КАРА СУПУРАСШУ" НО НУРИ Э О ПУРЭЗЭНТО! МАРИО ТАНЗАКУ О ЦУКУТТЭ МИЁУ! СУТАФФУ ДЖИКИДЭН!! МАРИО НО ИРАСУТО ГА ДЭКИРУ МАДЭ [СУПА МАРИО ШИРИЗУ Vol. 3] НИНТЭНДОКИЗЗУСУПЭСУ КАРА НУРИ Э ПУРЭЗЭНТО! [СУПА МАРИО ШИРИЗУ Vol. 2] НИНТЭНДОКИЗЗУСУПЭСУ КАРА НУРИ Э ПУРЭЗЭНТО! "СУПА МАРИО МЭКА (ВИИ У)" МАРИО НО ОРИДЖИНАРУКАБЭГАМИ О ЦУКУРОУ! ДАИ КОКАИ! МАРИО КЯРАБЭН НО ЦУКУРИКАТА МАРИО & РУИДЖИ АРУПИДЖИ ПЭПА МАРИО МИX НИ ТОДЖО СУРУ ДОДЭКАКУРАФУТО О ЦУКУТТЭ МИЁУ! ГЭМУДЭ ВА КОН'НА КАНДЖИ! ХАППЙ ХАЛЛОВЭЭН! МАРИО ТО РУИДЖИ НИ ХЭНСО ШИ ЧАОУ! НУРИ Э ПУРЭЗЭНТО [СУПА МАРИО ШИРИЗУ Vol. 1]
СУПА МАРИО МЭКА КОСУ САКУСЭИ КОЗА МАШИКО ТО ЯМАМУРА ТОШИНОСЭ-ХЭН ТЭНОХИРА САИЗУ НО ФАМИКОМ ТОДЖО! НАИЗО СОФУТО О ДАИ КОКАИ (1990 ~ 1993) ТЭНОХИРА САИЗУ НО ФАМИКОМ ТОДЖО! КИНОКО ОКОКУ НО КАКУРЭТА СУТА!? КИНОПИО ДАИ ТОКУШУ ТЭНОХИРА САИЗУ НО ФАМИКОМ ТОДЖО! НАИЗО СОФУТО О ДАИ КОКАИ (1983 ~ 1986) НИНТЭНДО НО ГЭМУ ТТЭ НИХОН ТО КАИГАИ ДЭ ДОКО ГА ЧИГАУ НО!? ХАНА-КУН & ФУДА-СЭНСЭИ НО ХАНАФУДА БАТОРУ ДОДЖО!! "КОИ-КОИ" О АСОНДЭ МИЁУ КОНО НАЦУ, РИО ДЭ АЦУКУНАРЭ! ХАНА-КУН & ФУДА-СЭНСЭИ НО ХАНАФУДА БАТОРУ ДОДЖО!! ХАНАФУДА ТТЭ НАНИ? СУПА МАРИО МЭКА КОСУ САКУСЭИ КОЗА МАШИКО ТО ЯМАМУРА БАНГАИ-ХЭН СОНО 2 СУПА МАРИО МЭКА КОСУ САКУСЭИ КОЗА МАШИКО ТО ЯМАМУРА БАНГАИ-ХЭН СОНО 1 РИО НО ШУЯКУ НИ ОДОРИДЭРО! ЧУ О МАИ, КЁДАИ НИ НАРУ. НАН ДЭМО АРИ НО ТЭНИСУ БАТОРУ! СУПА МАРИО МЭКА КОСУ САКУСЭИ КОЗА МАШИКО ТО ЯМАМУРА САИШУ-БАНАШИ СУПА МАРИО МЭКА КОСУ САКУСЭИ КОЗА МАШИКО ТО ЯМАМУРА ДАИ РОКУ ВА "ФАИНАРУ ФАНТАДЖИ VИИ" КАРА КУРА УДО САНСЭН!! СУПА МАРИО МЭКА КОСУ САКУСЭИ КОЗА МАШИКО ТО ЯМАМУРА ДАИ ГО ВА "ЧОИ ТЭКУ" СУБЭТЭ ВА КОКО КАРА УМАРЭРУ ЧО! [Vol. 7] СУПА МАРИО МЭКА КОСУ САКУСЭИ КОЗА МАШИКО ТО ЯМАМУРА ДАИ ЁН ВА СУПА МАРИО МЭКА КОСУ САКУСЭИ КОЗА МАШИКО ТО ЯМАМУРА ДАИ САН ВА СУПА МАРИО МЭКА КОСУ САКУСЭИ КОЗА МАШИКО ТО ЯМАМУРА ДАИ НИ ВА СУПА МАРИО МЭКА КОСУ САКУСЭИ КОЗА МАШИКО ТО ЯМАМУРА ДАИ ИЧИ ВА "ЧОИ ТЭКУ" КОТОШИ ВА, СУПА МАРИО 30 ШУНЭН НО ТОШИДА ЧО! [Vol. 6] ЧОИТЭ-КУН ГА ГЭМУ ШОППУ НИ ЯТТЭКИТА [Vol. 5] "ЧОИ ТЭКУ" МЭМЭМЭМЭМЭ СОРЭ, МЭГАТЭКУ~! [Vol. 4] АРЭ? ЧОИТЭ-КУН ГА, “НЭНДО” НИ НАКЧАТТА!! [Vol. 2] ДОМО. КОНО БА О О КАРИШИ ТЭ ЧОИ ТЭКУ О ХАДЖИМЭ ТЭ МИМАШИТА. [Vol. 1]
ДАИГАССО! БАНДО БУРАЗАЗУ П: МАНГА БАБАРА-ЧАН П БАБАРА & АШУРИ МАНГА БАБАРА-ЧАН П БАБАРА ТО ЯМАМУРА КАИХАЦУ СУТАФФУ ГА ЭГАКУ! СУПЭШАРУ КОМИККУ АШУРИ НО ХАРОВИН НАИТО СУСУМЭ! КИНОПИО ТАИЧО ДАИ 10 КАИ: АРАТАНАРУ БОКЭН СУСУМЭ! КИНОПИО ТАИЧО ДАИ 9 КАИ: ХАППИ ЭНДО? СУСУМЭ! КИНОПИО ТАИЧО ДАИ 8 КАИ: ПУРЭЗЭНТО СУСУМЭ! КИНОПИО ТАИЧО ДАИ 7 КАИ: КИНОПИО ТАИЧО КЮШУЦУ САКУСЭН СУСУМЭ! КИНОПИО ТАИЧО ДАИ 6 КАИ: ТОРОККО МАУНТЭН НИТЭ СУСУМЭ! КИНОПИО ТАИЧО ДАИ 5 КАИ: ВИНГО ТО ТАИКЭЦУ СУСУМЭ! КИНОПИО ТАИЧО ДАИ 4 КАИ: ХЭИХО НО МАЧИКАДО НИТЭ СУСУМЭ! КИНОПИО ТАИЧО ДАИ 3 КАИ: СУТАТО НО ХАНАШИ СУСУМЭ! КИНОПИО ТАИЧО ДАИ 2 КАИ: КОГЭН НО КИНОКО ИВА НИТЭ СУСУМЭ! КИНОПИО ТАИЧО ДАИ 1 КАИ: КЁРО-ХЭИ НО РОРУ ШИНДЭН НИТЭ
Planets according to Wikipedia
Mercury is the smallest planet in the Solar System and the closest to the Sun. Its orbit around the Sun takes 87.97 Earth days, the shortest of all the Sun's planets. It is named after the Roman god Mercurius (Mercury), god of commerce, messenger of the gods, and mediator between gods and mortals, corresponding to the Greek god Hermes (Ἑρμῆς). Like Venus, Mercury orbits the Sun within Earth's orbit as an inferior planet, and its apparent distance from the Sun as viewed from Earth never exceeds 28°. This proximity to the Sun means the planet can only be seen near the western horizon after sunset or the eastern horizon before sunrise, usually in twilight. At this time, it may appear as a bright star-like object, but is more difficult to observe than Venus. From Earth, the planet telescopically displays the complete range of phases, similar to Venus and the Moon, which recurs over its synodic period of approximately 116 days.
Mercury rotates in a way that is unique in the Solar System. It is tidally locked with the Sun in a 3:2 spin–orbit resonance,[17] meaning that relative to the fixed stars, it rotates on its axis exactly three times for every two revolutions it makes around the Sun.[a][18] As seen from the Sun, in a frame of reference that rotates with the orbital motion, it appears to rotate only once every two Mercurian years. An observer on Mercury would therefore see only one day every two Mercurian years.
Mercury's axis has the smallest tilt of any of the Solar System's planets (about 1⁄30 degree). Its orbital eccentricity is the largest of all known planets in the Solar System;[b] at perihelion, Mercury's distance from the Sun is only about two-thirds (or 66%) of its distance at aphelion. Mercury's surface appears heavily cratered and is similar in appearance to the Moon's, indicating that it has been geologically inactive for billions of years. Having almost no atmosphere to retain heat, it has surface temperatures that vary diurnally more than on any other planet in the Solar System, ranging from 100 K (−173 °C; −280 °F) at night to 700 K (427 °C; 800 °F) during the day across the equatorial regions.[19] The polar regions are constantly below 180 K (−93 °C; −136 °F). The planet has no known natural satellites.
Two spacecraft have visited Mercury: Mariner 10 flew by in 1974 and 1975; and MESSENGER, launched in 2004, orbited Mercury over 4,000 times in four years before exhausting its fuel and crashing into the planet's surface on April 30, 2015.[20][21][22] The BepiColombo spacecraft is planned to arrive at Mercury in 2025.
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 Earth's night sky after the Moon, Venus can cast shadows and can be visible to the naked eye in broad daylight.[18][19] Venus's orbit is smaller than that of Earth, but its maximal elongation is 47°; thus, at latitudes with a day-night cycle, it is most readily visible for up to a few hours following the start of sunset or before sunrise. At times, it has been seen in a completely dark sky. Venus orbits the Sun every 224.7 Earth days.[20] It has a synodic day length of 117 Earth days and a sidereal rotation period of 243 Earth days. Consequently, it takes longer to rotate about its axis than any other planet in the Solar System, and does so in the opposite direction to all but Uranus. This means that the Sun rises from its western horizon and sets in its east.[21] Venus does not have any moons, a distinction it shares only with Mercury among the planets in the Solar System.[22]
The third smallest planet in the Solar System, 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. It is radically different from Earth in other respects. It has the densest atmosphere of the four terrestrial planets, consisting of more than 96% carbon dioxide. The atmospheric pressure at the planet's surface is about 92 times the sea level pressure of Earth, or roughly the pressure at 900 m (3,000 ft) underwater on Earth. Even though Mercury is closer to the Sun, Venus has the hottest surface of any planet in the Solar System, with a mean temperature of 737 K (464 °C; 867 °F). Venus is shrouded by an opaque layer of highly reflective clouds of sulfuric acid, preventing its surface from being seen from Earth in light. It may have had water oceans in the past,[23][24] but after these evaporated the temperature rose under a runaway greenhouse effect.[25] The water has probably photodissociated, and the free hydrogen has been swept into interplanetary space by the solar wind because of the lack of a planetary magnetic field.[26] Because of the lethal surface conditions, the planet is sometimes referred to as Earth's "evil twin".[27]
As one of the brightest objects in the sky, Venus has been a major fixture in human culture for as long as records have existed. It has been made sacred to gods of many cultures and has been a prime inspiration for writers and poets as the "morning star" and "evening star". Venus was the first planet to have its motions plotted across the sky, as early as the second millennium BCE.[28]
Its proximity to Earth has made Venus a prime target for early interplanetary exploration. It was the first planet beyond Earth visited by a spacecraft (Venera 1 in 1961) and the first to be successfully landed on (by Venera 7 in 1970). The planet's thick clouds render observation of its surface impossible in the visible spectrum, and the first detailed maps did not emerge until the arrival of the Magellan orbiter in 1991. Plans have been proposed for rovers or more complex missions, but they are hindered by Venus's hostile surface conditions. The possibility of life on Venus has long been a topic of speculation; in recent years, the topic has received active research.
Earth is the third planet from the Sun and the only astronomical object known to harbor life. While large volumes of water can be found throughout the Solar System, only Earth sustains liquid surface water. About 71% of Earth's surface is made up of the ocean, dwarfing Earth's polar ice, lakes, and rivers. The remaining 29% of Earth's surface is land, consisting of continents and islands. Earth's surface layer is formed of several slowly moving tectonic plates, interacting to produce mountain ranges, volcanoes, and earthquakes. Earth's liquid outer core generates the magnetic field that shapes Earth's magnetosphere, deflecting destructive solar winds.
Earth's atmosphere consists mostly of nitrogen and oxygen. More solar energy is received by tropical regions than polar regions and is redistributed by atmospheric and ocean circulation. Water vapor is widely present in the atmosphere and forms clouds that cover most of the planet. Greenhouse gases in the atmosphere like carbon dioxide (CO2) trap a part of the energy from the Sun close to the surface. A region's climate is governed by latitude, but also by elevation and proximity to moderating oceans. Severe weather, such as tropical cyclones, thunderstorms, and heatwaves, occurs in most areas and greatly impacts life.
Earth is an ellipsoid with a circumference of about 40,000 km. It is the densest planet in the Solar System. Of the four rocky planets, it is the largest and most massive. Earth is about eight light minutes away from the Sun and orbits it, taking a year (about 365.25 days) to complete one revolution. Earth rotates around its own axis in slightly less than a day (in about 23 hours and 56 minutes). Earth's axis of rotation is tilted with respect to the perpendicular to its orbital plane around the Sun, producing seasons. Earth is orbited by one permanent natural satellite, the Moon, which orbits Earth at 380,000 km (1.3 light seconds) and is roughly a quarter as wide as Earth. The Moon always faces the Earth with the same side through tidal locking and causes tides, stabilizes Earth's axis, and gradually slows its rotation.
Earth formed over 4.5 billion years ago. During the first billion years of Earth's history, the ocean formed and then life developed within it. Life spread globally and began to affect Earth's atmosphere and surface, leading to Earth's Great Oxidation Event two billion years ago. Humans emerged 300,000 years ago, and have reached a population of almost 8 billion today. Humans depend on Earth's biosphere and natural resources for their survival, but have increasingly impacted Earth's environment. Today, humanity's impact on Earth's climate, soils, waters, and ecosystems is unsustainable, threatening people's lives and causing widespread extinction of other life.
Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System, being larger than only Mercury. In the English language, Mars is named for the Roman god of war. Mars is a terrestrial planet with a thin atmosphere, and has a crust primarily composed of elements similar to Earth's crust, as well as a core made of iron and nickel. Mars has surface features such as impact craters, valleys, dunes, and polar ice caps. It has two small and irregularly shaped moons: Phobos and Deimos.
Some of the most notable surface features on Mars include Olympus Mons, the largest volcano and highest known mountain on any planet in the Solar System, and Valles Marineris, one of the largest canyons in the Solar System. The Borealis basin in the Northern Hemisphere covers approximately 40% of the planet and may be a large impact feature.[19] Days and seasons on Mars are comparable to those of Earth, as the planets have a similar rotation period and tilt of the rotational axis relative to the ecliptic plane. Liquid water on the surface of Mars cannot exist due to low atmospheric pressure, which is less than 1% of the atmospheric pressure on Earth.[20][21] Both of Mars's polar ice caps appear to be made largely of water.[22][23] In the distant past, Mars was likely wetter, and thus possibly more suited for life. However, it is unknown whether life has ever existed on Mars.
Mars has been explored by several uncrewed spacecraft, beginning with Mariner 4 in 1965. NASA's Viking 1 lander transmitted in 1976 the first images from the Martian surface. Two countries have successfully deployed rovers on Mars, the United States first doing so with Sojourner in 1997 and China with Zhurong in 2021.[24] There are also planned future missions to Mars, such as a Mars sample-return mission set to happen in 2026, and the Rosalind Franklin rover mission, which was intended to launch in 2018 but was delayed to 2024 at the earliest, with a more likely launch date at 2028.
Mars can be viewed from Earth with the naked eye, as can its reddish coloring. This appearance, due to the iron oxide prevalent on its surface, has led to Mars often being called the Red Planet.[25][26] It is among the brightest objects in Earth's sky, with an apparent magnitude that reaches −2.94, comparable to that of Jupiter and surpassed only by Venus, the Moon and the Sun.[14] Historically, Mars has been observed since ancient times, and over the millennia, has been featured in culture and the arts in ways that have reflected humanity's growing knowledge of it.
