Iouik

Iothalamic acid

Iotape Philadelphus

Iota Sigma Pi (ΙΣΠ) is a national honor society in the United States. It was established in 1902 and specializes in the promotion of women in the sciences, especially chemistry. It also focuses on personal and professional growth for women in these fields. As with all honor societies, they create professional networks along with recognizing achievements of women in chemistry.

Iota Geminorum in fiction

Iota Horologii b (ι Hor b / ι Horologii b), often catalogued HR 810 b, is an extrasolar planet approximately 56 light-years away in the constellation of Horologium (the Pendulum Clock). Iota Horologii b has a minimum mass 1.94 times that of Jupiter, however preliminary astrometric measurements suggest that the object may be around 24 Jupiter masses and would therefore be a brown dwarf.

ι Leonis

Iota Pictoris (ι Pictoris) is a binary star system in the Pictor constellation.The brighter star, Iota Pictoris A, is an F0V star with apparent magnitude about 5.61, while the dimmer star, Iota Pictoris B, is a cooler F4V star with apparent magnitude about 6.24. They are separated by about 12.9", about 500 AU.

Iotti

Ioudaios (Ancient Greek: Ἰουδαῖος; pl. Ἰουδαῖοι Ioudaioi) is an Ancient Greek ethnonym used in classical and biblical literature which commonly translates to "Jew" or "Judean".The choice of translation is the subject of frequent scholarly debate, given its central importance to passages in the Bible (both the Hebrew Bible and the New Testament) as well as works of other writers such as Josephus and Philo.

Ioulia Timonova

The Bayer designation Iota Cygni (ι Cyg / ι Cygni) is shared by two stars, in the constellation Cygnus:ι¹ Cygni, dimmer (magnitude 5.75)ι² Cygni, brighter (magnitude 3.77), often simply called ι Cyg

Iota Orion

Iota Carinae (ι Carinae, abbreviated Iota Car, ι Car), also named Aspidiske, is a star in the southern circumpolar constellation (circumpolar if viewed at any location from approximately 40° S to the South Pole) of Carina. With an apparent visual magnitude of 2.2, it is one of the brighter stars in the night sky. It can be seen from the latitude of Alexandria or Mobile, Alabama and southward.The False Cross is an asterism formed from Iota Carinae, Delta Velorum, Kappa Velorum and Epsilon Carinae. It is so called because it is sometimes mistaken for the Southern Cross, causing errors in astronavigation.

Iota ringtail

Iota Apodis (ι Aps, ι Apodis) is the Bayer designation for a binary star system in the southern circumpolar constellation of Apus. It is a faint target at an apparent visual magnitude of 5.41, but still visible to the naked eye from suitably dark skies.

Iota Reticuli

Iota Telescopii (ι Telescopii) is a solitary, orange-hued star in the southern constellation of Telescopium. It is a K-type giant star of spectral type K0 III with an apparent magnitude of +4.89. Around 164 times as luminous as the Sun, it is approximately 370 light years from Earth.

Iotaphora

ι Geminorum

Iotapian

The Iouanga River is a river of New Caledonia. It has a catchment area of 522 square kilometres.

Iota Cephei (ι Cephei, ι Cep) is a solitary star in the northern constellation Cepheus. Based upon an annual parallax shift of 15.83 mas as seen from the Earth, it is located about 206 light years from the Sun. The star is visible to the naked eye with an apparent visual magnitude of 3.5.This is a K-type giant star with a stellar classification of K0 III. It is currently at an evolutionary stage known as a red clump, indicating that it is generating energy through the fusion of helium at its core. This star has 11 times the Sun's radius and about 2.15 times the mass of the Sun. It is emitting 57 times as much luminosity as the Sun, which is being radiated from its photosphere at an effective temperature of 4,768 K.

Iotapa (who lived in the 1st century) was a daughter of King Sampsiceramus II of Emesa who married the Herodian Prince Aristobulus Minor.

Iota Volantis (ι Vol, ι Volantis) is the Bayer designation for a star in the southern constellation of Volans. It has an apparent visual magnitude of 5.39, which indicates it is faintly visible to the naked eye. With a parallax of 0.00579″, it lies at an estimated distance of roughly 560 light years from the Sun.This star has a stellar classification of B7 III, which means it is a B-type giant star.

*Metrocampa admirabilis (Oberthur, 1884)

Iotyrris musivum is a species of sea snail, a marine gastropod mollusk in the family Turridae, the turrids.

Iota Crateris (ι Crt) is the Bayer designation for a binary star system in the southern constellation of Crater. It is faintly visible to the naked eye with an apparent visual magnitude of 5.48. According to the Bortle scale, this means it can be viewed from suburban skies at night. Based upon an annual parallax shift of 37.41 mas, Iota Crateris is located 87 light years from the Sun.This is an astrometric binary system with an estimated orbital period of roughly 79,000 years.

Iothalmate

Iotapa (daughter of Sampsiceramus II)

Iota Draconis b, also named Hypatia, is an exoplanet orbiting the K-type giant star Iota Draconis about 101.2 light-years (31 parsecs, or nearly 2.932×1014 km) from Earth in the constellation Draco. The exoplanet was found by using the radial velocity method, from radial-velocity measurements via observation of Doppler shifts in the spectrum of the planet's parent star. It was the first planet discovered orbiting a giant star.Following its discovery the planet was designated Iota Draconis b. In July 2014 the International Astronomical Union launched a process for giving proper names to certain exoplanets and their host stars. The process involved public nomination and voting for the new names. In December 2015, the IAU announced that the winning name for this planet was Hypatia. The winning name was submitted by Hypatia, a student society of the Physics Faculty of the Universidad Complutense de Madrid, Spain. Hypatia was a famous Greek astronomer, mathematician, and philosopher.

Iota² Scorpii

Iouik, also spelled Iwik, is a coastal town in western Mauritania. Located in the Banc d'Arguin National Park within the Dakhlet Nouadhibou region, it sits on a small peninsula.Nearby towns and villages include Uad Guenifa (73.4 nm), Cansado (72.0 nm), Tanoudert (21.5 nm), Akjoujt (108.4 nm), El Mamghar (32.4 nm), Regbet Thila (28.6 nm) and Tikattane (50.1 nm) .Iouik is very close to the island of Tidra lying in the southwest some 3 km distant, further west is Niroumi and around 10 km north are the Kiaone islands.

Iota Persei (Iota Per, ι Persei, ι Per) is a main sequence dwarf star in the constellation Perseus. It is somewhat larger and greater in mass than the Sun, and is located about 34 light years distant. Iota Persei has a relatively high proper motion across the sky, and moves at a net velocity of 92 km/s, relative to the Sun.No sub-stellar companions to this star have yet been found. There is a 12th-magnitude line-of-sight companion star that is not believed to be gravitationally associated with Iota Persei.

Iothia radiata is a species of sea snail, a true limpet, a marine gastropod mollusk in the family Lepetidae, one of the families of true limpets.

Iouea

Iota Ophiuchi

Iou Dam

Iouga is a suggested reconstruction of the name of a Romano-British goddess known from a single fragmentary inscription on an altar-stone at York.

Iotated E (Ѥ ѥ) is a letter of the Cyrillic script. It is no longer used in any modern language.

ι Lyrae, Latinised as Iota Lyrae, is a binary star in the constellation Lyra. Its apparent magnitude is 5.22. Located around 275 parsecs (900 ly) distant, it is composed of a blue subgiant primary of spectral type B6IV and an unknown secondary separated by 0.08 arcseconds.

Iotified A

Iota High School

Iota Leporis (ι Leporis) is a triple star system in the southern constellation of Lepus. It is visible to the naked eye as a point source of blue-white light with an apparent visual magnitude of 4.45.

Iota Crateris (ι Crt) is the Bayer designation for a binary star system in the southern constellation of Crater. It is faintly visible to the naked eye with an apparent visual magnitude of 5.48. According to the Bortle scale, this means it can be viewed from suburban skies at night. Based upon an annual parallax shift of 37.41 mas, Iota Crateris is located 87 light years from the Sun.This is an astrometric binary system with an estimated orbital period of roughly 79,000 years. The primary, component A, is an F-type main sequence star with a stellar classification of F6.5 V, which is generating energy through the thermonuclear fusion of hydrogen in its core region. It is around 4.45 billion years old with 1.19 times the mass of the Sun. The star is radiating energy from its outer atmosphere at an effective temperature of 6,230 K.The companion, component B, is a red dwarf star with a probable classification of M3, although its mass estimate of 0.57 solar would be more consistent with an M0 class star. As of 2014, this magnitude 11.0 star had an angular separation of 1.10 arc seconds along a position angle of 248°. It has a projected separation of 25 AU, which means it is positioned at least this distance away from the primary.

Iota Trianguli

Iotated A (Cyrillic)

Iota Pictoris

Iota Horologii

Iothia

Iotapa (born around 20 BC-unknown date of death) was a princess of Commagene, daughter of King Mithridates III of Commagene, Queen consort of Syrian King Sampsiceramus II of Emesa.

Iota Telescopii

Iota Orionis

Iota Tucanae

Ioueldaob (sometimes spelled Eoueldaob) is a region in the Republic of Palau located south of the island of Babeldaob. It includes the islands within the State of Koror, the states of Peleliu and Angaur. It is a traditional division between the northern and the southern islands. Ioueldaob literally means "lower sea", while Babeldaob means "upper sea".
Ioueldaob

Iota Ursae Majoris (ι Ursae Majoris, abbreviated Iota UMa, ι UMa), also named Talitha, is a star system in the northern circumpolar constellation of Ursa Major. It has an apparent visual magnitude of 3.14, making it visible to the naked eye and placing it among the brighter members of this constellation. Based upon parallax measurements, it is located at a distance of 47.3 light-years (14.5 parsecs) from the Sun.

Iota Chamaeleontis

Iota Piscis Austrini (ι Piscis Austrini) is a solitary, blue-white hued star in the southern constellation of Piscis Austrinus. It has an apparent visual magnitude of +4.35 and is around 500 light years from the Sun. This is an A-type main sequence star with a stellar classification of A0 V. It has a magnitude 11.4 visual companion located at an angular separation of 20 arc seconds along a position angle of 290°, as of 1910.Iota Piscis Austrini is moving through the Galaxy at a speed of 29.7 km/s relative to the Sun. Its projected Galactic orbit carries it between 18,400 and 24,300 light years from the center of the Galaxy.

Iotapa (spouse of Sampsiceramus II)

*Patella emarginuloides( Philippi, 1868)

Iotatorquevirus is a recently discovered genus in the new family of Anelloviridae, in group II in the Baltimore classification. It encompasses the two type species of the Torque Teno Sus Virus 1 and 2.

Iota Hydrae

Iota Herculis (ι Her, ι Herculis) is a fourth-magnitude variable star in the constellation Hercules.

Iota Piscium (Iota Psc, ι Piscium, ι Psc) is single, F-type main-sequence star located 45 light years from Earth, in the constellation Pisces. Its spectral type is F7V, which means that it is somewhat larger and brighter than the Sun, but still within the range considered to have the potential for Earth-like planets. It has a surface temperature of about 6,000 to 7,500 K.

Iota Phi Theta Fraternity, Inc.

Iotuba chengjiangensis is a problematic Cambrian fossil with a U-shaped gut and tentacles, known from the Chengjiang biota. Originally interpreted as a phoronid, its affinity is currently disputed. It, and the possibly-synonymous taxon Eophoronis, resemble the 'priapulid' Louisella.

Iota Leporis

Iota Volantis (ι Vol, ι Volantis) is the Bayer designation for a star in the southern constellation of Volans. It has an apparent visual magnitude of 5.39, which indicates it is faintly visible to the naked eye. With a parallax of 0.00579″, it lies at an estimated distance of roughly 560 light years from the Sun.This star has a stellar classification of B7 III, which means it is a B-type giant star. However, some sources give it a classification of B7 IV, which would indicate it is a subgiant star. It has 3.7 times the mass of the Sun and is spinning rapidly with a projected rotational velocity of 129 km/s. The estimated size of the star is 4.7 times the radius of the Sun, and it shines with around 313 times the Sun's luminosity. The effective temperature of the star's outer atmosphere is 11,803 K, giving it the blue-white hue of a B-type star.

Iota Piscis Austrini

Iotified big yus

Iotapa (born in 43 BC-unknown date of death) was a princess of Media Atropatene, daughter of King Artavasdes I of Media Atropatene. She was Queen consort of King Mithridates III of Commagene.

Iotabrycon praecox

Iotapianus

Iotalamic acid

Iota Capricorni (ι Cap, ι Capricorni) is a solitary, yellow-hued star in the southern constellation of Capricornus. It can be seen with the naked eye, having an apparent visual magnitude of +4.3. Based upon an annual parallax shift of 16.58 mas as seen from the Earth, the star is located about 197 light years from the Sun.

Iotated E

ι Phoenicis

Iota, Jot, Zot

Ioudaion

ι Lupi

Iouanga River

Iota Gruis

Iotyrris devoizei

Iota Island is an island of Bermuda located in Warwick Parish.

Iota Piscium (Iota Psc, ι Piscium, ι Psc) is single, F-type main-sequence star located 45 light years from Earth, in the constellation Pisces. Its spectral type is F7V, which means that it is somewhat larger and brighter than the Sun, but still within the range considered to have the potential for Earth-like planets. It has a surface temperature of about 6,000 to 7,500 K. Iota Piscium is a suspected to be a variable star, and was once thought to have one or two stellar companions, but both are line-of-sight coincidences. It displays a far-infrared excess at a wavelength of 70μm, suggesting it is being orbited by a cold debris disk.

Iota Reticuli (ι Reticuli) is a solitary, orange-hued star in the southern constellation of Reticulum. It is faintly visible to the naked eye, having a combined apparent visual magnitude of +4.97. Based upon an annual parallax shift of 10.22 mas as seen from Earth, it is located around 319 light years from the Sun. This is an evolved K-type giant star with a stellar classification of K4 III.Iota Reticuli is moving through the Galaxy at a speed of 80.9 km/s relative to the Sun.

Iota¹ Scorpii

Iouga

Iota High School is a high school located in Iota, Louisiana, United States. The school is a part of the Acadia Parish School Board.

Iota Sagittarii

Iota Horologii c

Ioujimae Station

ι Lupi, Latinised as Iota Lupi, is a solitary star in the southern constellation of Lupus. It is visible to the naked eye with an apparent visual magnitude of 3.54. Based upon an annual parallax shift of 9.65 mas as seen from Earth, it is located around 338 light years from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.23 due to interstellar dust. Relative to its neighbors, this star has a peculiar velocity of 27.4±4.9 km/s.

Iotaphora is a genus of moth in the family Geometridae.

Ioto

ι Ophiuchi

Iotification

Iota Carinae (ι Carinae, abbreviated Iota Car, ι Car), also named Aspidiske, is a star in the southern circumpolar constellation (circumpolar if viewed at any location from approximately 40° S to the South Pole) of Carina. With an apparent visual magnitude of 2.2, it is one of the brighter stars in the night sky.

Iotified

ι Carinae

ι Sculptoris

Iota Draconisb

Iotyrris

Iota Nu Delta (ΙΝΔ, also IND) is the first South Asian interest college fraternity. IND was founded in 1994 at the Binghamton University. It is a member of the North-American Interfraternity Conference since 2007 and National APIA Panhellenic Association since 2016.

Iota Capricorni

Iota Eta

Iotified small yus

Iotabrycon praecox is a species of characin endemic to Ecuador, where it is found in the Vinces River basin. This species is the only member of its genus.

Iota Leonis

Iothia radiata

Iota Apodis

Iota Volantis

* Xenuroturris cingulifera (Lamarck, 1822)

Iota Persei in fiction

Iothia emarginuloides

Iotapa (born around 20 BC), a daughter of King Mithridates III of Commagene, reigned as Queen of Commagene after marrying her King brother Antiochus III.

Iota Muscae

Iotyrris cingulifera is a species of sea snail, a marine gastropod mollusk in the family Turridae, the turrids.

Iotapapillomavirus is a genus of viruses, in the family Papillomaviridae. Rodents serve as natural hosts. There are currently only one species in this genus: the type species Iotapapillomavirus 1. Diseases associated with this genus include: cutaneous lesions and benign skin tumours, such as papillomas and keratoacanthomas.

Iotyrris cingulifera

Iota Tucanae (ι Tuc, ι Tucanae) is a solitary star in the southern constellation of Tucana. Based upon an annual parallax shift of 10.72 mas as seen from Earth, it is located around 304 light years from the Sun. With an apparent visual magnitude of +5.33, it is faintly visible to the naked eye.This is a yellow-hued G-type giant star with a stellar classification of G5 III.

Iotating

Ioukhtas

Iotatorquevirus

Iota Horologii in fiction

Iothia emarginuloides is a species of sea snail, a true limpet, a marine gastropod mollusk in the family Lepetidae, one of the families of true limpets. This species was previously known as Iothia coppingeri.

Iotapa (disambiguation)

ι Eridani

Ioulia Chtchetinina

Iotapa (spouse of Antiochus III)

Iota Hydrae, Latinized from ι Hydrae, is a star in the constellation Hydra, about 8° to the north-northwest of Alphard and just to the south of the celestial equator. Visible to the naked eye, it is a suspected variable star with an apparent visual magnitude that ranges between 3.87 and 3.91. Based upon an annual parallax shift of 12.39 mas, it is located around 263 light years from the Sun.This is an evolved K-type giant star with a stellar classification of K2.5 III. It is a Barium star, which means that, for a giant star, it displays unusually strong absorption lines of singly-ionized barium and strontium. Iota Hydrae has nearly twice the mass of the Sun and has expanded to 33 times the Sun's radius. It is around 2.5 billion years old and is spinning with a leisurely projected rotational velocity of 4.5 km/s. It may be a member of the Wolf 630 moving group of stars that share a common trajectory through space.

Iotated vowel

Iota Phi Lambda Sorority Inc. (ΙΦΛ) is the first African American Greek-lettered business sorority established by African American business women. There are now more than 100 chapters with membership numbering more than 5,000 in 85 cities and the US Virgin Islands. Iota Phi Lambda is not an NPHC sorority and dual membership within Iota Phi Lambda Sorority and NPHC sororities is allowed.

Iota Apodis (ι Aps, ι Apodis) is the Bayer designation for a binary star system in the southern circumpolar constellation of Apus. It is a faint target at an apparent visual magnitude of 5.41, but still visible to the naked eye from suitably dark skies. The distance to this star can be roughly gauged from parallax measurements, yielding an estimate of 1,300 light-years (400 parsecs) with a 20% margin of error.Both stars are B-type main sequence stars, which indicates they shine with a blue-white hue. The brighter component has a stellar classification of B9 V and an apparent magnitude 5.90, while the second member is a B9.5 V star with a magnitude of 6.46. The pair have an angular separation of 0.091 arcseconds with an estimated orbital period of 59.32 years. They are about 3.89 and 3.45 times as massive as the Sun.

Iota Delphini (ι Del, ι Delphini) is a star in the constellation Delphinus. It has an apparent magnitude of about 5.4, meaning that it is just barely visible to the naked eye. Based upon parallax measurements made by the Hipparcos spacecraft, this star is around 177 light years away from the Sun.Iota Delphini's spectral type is A1IV, meaning it is an A-type subgiant. Observations of the star's spectrum reveal a periodic Doppler shift. This means that Iota Delphini is a spectroscopic binary with a period of 11 days and an eccentricity of 0.23. However, almost no information is known about the companion star.Iota Delphini appears to be an Am star, also known as an metallic-line star. These types of stars have spectra indicating varying amounts of metals, like iron. Observations of Iota Delphini's spectrum have showed lower amounts of calcium and higher amounts of iron than usual.

Iota Phi Theta Fraternity, Incorporated (ΙΦΘ) is a nationally incorporated, historically African-American, collegiate fraternity whose purpose is the development and perpetuation of Scholarship, Leadership, Citizenship, Fidelity and Brotherhood among Men. It was founded on September 19, 1963, at Morgan State University (then Morgan State College) in Baltimore, Maryland. At present, it consists of over 70,000 members.

Iota Reticuli (ι Reticuli) is a solitary, orange-hued star in the southern constellation of Reticulum. It is faintly visible to the naked eye, having a combined apparent visual magnitude of +4.97. Based upon an annual parallax shift of 10.22 mas as seen from Earth, it is located around 319 light years from the Sun. This is an evolved K-type giant star with a stellar classification of K4 III.Iota Reticuli is moving through the Galaxy at a speed of 80.9 km/s relative to the Sun. Its projected Galactic orbit carries it between 12,300 and 25,100 light years from the center of the Galaxy.Iota Reticuli came closest to the Sun 883,000 years ago when it had brightened to magnitude 4.08 from a distance of 212 light years.

Ioulia Chtchetinina (Russian: Юлия Щетинина; born 24 December 1995) is a pair skater who competes for Switzerland. With Noah Scherer, she won three international medals and competed at two World Championships. In mid-May 2017, the Swiss skating federation announced that they had parted ways, and she competed the 2017–2018 season with Mikhail Akulov.

Iotuba

Iota Pegasi (ι Peg, ι Pegasi) is a star located within the constellation Pegasus. It is about 38 light-years from Earth. It is a spectroscopic binary system.Iota Pegasi A is a yellowish-white star somewhat brighter than the sun. It and the dimmer Iota Pegasi B orbit each other with a period of about 10 days. In about four billion years from now, component A will evolve off the main sequence into a giant. In the process it will overflow its Roche lobe and begin to transfer mass onto the secondary. This may cause the secondary to acquire enough mass to become the primary component. After both stars have passed through the giant star stage, the end result will be a pair of co-orbiting white dwarfs in about eight billion years.

Iotaphora admirabilis

Iotrolan

Iothia fulva

Iota Crucis, Latinized from ι Crucis, is a star in the constellation Crux. It has an apparent magnitude of 4.69m. The star is classified as an orange giant (spectral class K1 III). Iota Crucis is located at 125 light-years from the Sun.There is a nearby 10.3m class G8 star, but the highly different proper motion reveals it to be a mere line-of-sight optical companion.

Ioudenitch

Iotyrris musivum

Iota Delphini (ι Del, ι Delphini) is a star in the constellation Delphinus. It has an apparent magnitude of about 5.4, meaning that it is just barely visible to the naked eye. Based upon parallax measurements made by the Hipparcos spacecraft, this star is around 177 light years away from the Sun.Iota Delphini's spectral type is A1IV, meaning it is an A-type subgiant. Observations of the star's spectrum reveal a periodic Doppler shift.

Iota Geminorum

Iotyrris cerithiformis is a species of sea snail, a marine gastropod mollusk in the family Turridae, the turrids.

Iotalamic acid (also iothalamic acid in USAN) and its salts (INN Iothalamates) is an iodine-containing organic anion used as a radiocontrast agent. It is available as sodium iothalamate (Iothalamate sodium) and meglumine iothalamate (Iothalmate meglumine). It can be administered intravenously or intravesically (into the urinary bladder).Radioactive formulation is also available as sodium iothalamate I-125 Injection (GLOFIL-125). It is indicated for evaluation of glomerular filtration in the diagnosis or monitoring of patients with renal disease.

Iothario

Iota Sculptoris (ι Scl) is a class K0III (orange giant) star in the constellation Sculptor. Its apparent magnitude is 5.18 and it is approximately 330 light years away from Earth based on parallax.

Iotyrris marquesensis

Iota Draconis b, also named Hypatia, is an exoplanet orbiting the K-type giant star Iota Draconis about 101.2 light-years (31 parsecs, or nearly 2.932×1014 km) from Earth in the constellation Draco. The exoplanet was found by using the radial velocity method, from radial-velocity measurements via observation of Doppler shifts in the spectrum of the planet's parent star. It was the first planet discovered orbiting a giant star.Following its discovery the planet was designated Iota Draconis b.

Ioujimae

In formal language theory and computer science, Iota and Jot (from Greek iota ι, Hebrew yodh י, the smallest letters in those two alphabets) are languages, extremely minimalist formal systems, designed to be even simpler than other more popular alternatives, such as the lambda calculus and SKI combinator calculus.

Iota Boötis

ι Orionis

Iota Eridani (ι Eri) is a solitary star in the constellation Eridanus. It is visible to the naked eye with an apparent magnitude of 4.11. With an annual parallax shift of 0.02165 arcseconds, it lies at an estimated distance of about 151 light years.This is a evolved red clump giant star with a stellar classification of K0 III. The measured angular diameter, after correcting for limb darkening, is 2.18±0.02 mas.

Ioulia Petrova

Iota Trianguli Australis (ι Trianguli Australis) is a binary star system in the constellation Triangulum Australe. It is visible to the naked eye with a combined apparent visual magnitude of +5.27. Based upon an annual parallax shift of 25.77 mas as seen from the Earth, it is located around 127 light years from the Sun. The system appears to be moving closer to the Sun with a radial velocity of around −6 km/s.

Iota Hydrae, Latinized from ι Hydrae, is a star in the constellation Hydra, about 8° to the north-northwest of Alphard and just to the south of the celestial equator. Visible to the naked eye, it is a suspected variable star with an apparent visual magnitude that ranges between 3.87 and 3.91. Based upon an annual parallax shift of 12.39 mas, it is located around 263 light years from the Sun.This is an evolved K-type giant star with a stellar classification of K2.5 III.

Iota Phi Theta

Iota Psc

Iota Sagittarii (Iota Sgr, ι Sagittarii, ι Sgr) is a star in the zodiac constellation of Sagittarius. With an apparent visual magnitude of +4.118, it is bright enough to be viewed with the naked eye. Based upon an annual parallax shift of 17.94 mas as seen from Earth, this star is located 182 light years from the Sun. It is moving away from the Earth with a radial velocity of +35.8 km/s.This is a probable astrometric binary, based upon proper motion data collected during the Hipparcos mission.

Ioudaizontes

Iotichthys phlegethontis

Iota Pegasi

Iothocera tomentosa

Iota Trianguli Australis

Iota Beta Chi (ΙΒΧ) is a Canadian national sorority. There are two active chapters in Atlantic Canada to date; one in Halifax, Nova Scotia, and the other in Fredericton, New Brunswick. Between these two chapters their membership totals over 300 members.There are three different divisions of Iota Beta Chi: the active chapters which recruit and are run by undergraduate members; the alumnae chapters which are made of Iota Beta Chi alumnae; and the Headquarters, which is composed of volunteering members of Iota Beta Chi's alumnae.

Iotic

Iotated A (Ꙗ, ꙗ) is a letter of the Cyrillic script, used today only in Church Slavonic. It is unusual among early Cyrillic letters in having no direct counterpart in Glagolitic: Ⱑ (jat’) is used for both /ě/ and /ja/. Accordingly, many early Cyrillic texts (particularly those with Glagolitic antecedents) may use Ѣ for both these purposes; this practice continues into the fourteenth century, but is much more common in the South Slavonic than the East Slavonic area. Nevertheless, Ꙗ is attested in the earliest extant Cyrillic writings, including for example the Codex Suprasliensis and Savvina Kniga.It continued in use in Serbian until the orthographical reforms of Vuk Karadžić, and in Bulgarian (where it also acquired a civil script glyph variant) until the late nineteenth century. Among the Eastern Slavs, the denasalisation of [ę], probably to [æ], and the subsequent coalescence of this sound with the /a/ phoneme meant that the letter Ѧ acquired the same function as Ꙗ, and the two came to be regarded as variants of the same letter. This is still the case in modern Church Slavonic, where, broadly speaking, Ꙗ is used initially and Ѧ elsewhere, though exceptionally they may be used to make other distinctions, such as that between ѧ҆зы́къ 'tongue' and ꙗ҆зы́къ 'people'.
Iotated A

ι Persei

Iotyrris cerithiformis

Iota Geminorum (ι Gem, ι Geminorum) is a solitary fourth-magnitude star in the constellation Gemini. In the sky, it forms an isosceles triangle with Castor and Pollux, and is located less than a degree from the 5th magnitude stars 64 and 65 Geminorum. It is called by the proper name Propus, meaning "forefoot" in Latin.In Chinese, 五諸侯 (Wu Zhū Hóu), meaning Five Feudal Kings, refers to an asterism consisting of ι Geminorum, θ Geminorum, τ Geminorum, υ Geminorum and φ Geminorum. Consequently, ι Geminorum itself is known as 五諸侯三 (Wu Zhū Hóu sān, English: the Third Star of Five Feudal Kings.).

Iota Cephei

Iotkt

Iotroxic acid

Iota Ursae Majoris

Iotified a

Lolita Lymoura

Iota Hor

Iota Delphini

Iota Coronae Borealis

*Iothia coppingeri magellanica( Linse, 2002)

Iota Leonis, Latinized from ι Leonis, is a triple star system in the constellation Leo. The system is fairly close to the Sun, at only 79 light-years (24.2 parsecs) away, based on its parallax. The system has a combined apparent magnitude of 4.00 making it faintly visible to the naked eye. It is moving closer to the Sun with a radial velocity of −10 km/s.Iota Leonis has a spectral type of F3 IV, matching that of an F-type subgiant star. It is a spectroscopic binary, which means it is a binary star with components that are too close together to be able to resolve individually through a telescope. In this case, light from only the primary star can be detected, and it is considered single-lined.The third component in the star system is designated Iota Leonis B. It orbits the central pair almost every 200 years, and with its perihelion passage in 1948, the separation between the two is steadily growing. Iota Leonis B has a mass approximately 8% greater than that of the Sun. It is a G-type main-sequence star, like the Sun.

Iota Tucanae (ι Tuc, ι Tucanae) is a solitary star in the southern constellation of Tucana. Based upon an annual parallax shift of 10.72 mas as seen from Earth, it is located around 304 light years from the Sun. With an apparent visual magnitude of +5.33, it is faintly visible to the naked eye.This is a yellow-hued G-type giant star with a stellar classification of G5 III. It is classified as a semiregular variable star, showing a periodicity of 66.8 days with an amplitude of 0.0202 in visual magnitude. Iota Tucanae is an X-ray source with a luminosity of 817.6×1028 erg s−1. It has an estimated 2.2 times the mass of the Sun, and, at the age of 1.69 billion years, it has evolved away from the main sequence, expanding to 11 times the Sun's radius. The star radiates 65 times the solar luminosity from its photosphere at an effective temperature of 5,039 K.

ι Cassiopeiae

Iota Persei (Iota Per, ι Persei, ι Per) is a main sequence dwarf star in the constellation Perseus. It is somewhat larger and greater in mass than the Sun, and is located about 34 light years distant. Iota Persei has a relatively high proper motion across the sky, and moves at a net velocity of 92 km/s, relative to the Sun.No sub-stellar companions to this star have yet been found.

* Pleurotoma cingulifera (Lamarck, 1822) (basionym)

Iota operator

Iotacism

Iota Pegasi (ι Peg, ι Pegasi) is a star located within the constellation Pegasus. It is about 38 light-years from Earth. It is a spectroscopic binary system.Iota Pegasi A is a yellowish-white star somewhat brighter than the sun. It and the dimmer Iota Pegasi B orbit each other with a period of about 10 days. In about four billion years from now, component A will evolve off the main sequence into a giant.

Iounane (Berber: ⵉⵢⵓⵏⴰⵏ, Transcription: iyunan) is a small town and rural commune in Chefchaouen Province of the Tangier-Tétouan region of Morocco. At the time of the 2004 census, the commune had a total population of 23132 people living in 3085 households.

Iotisis is a genus of deep-sea bamboo coral in the family Isididae. It is monotypic with a single species, Iotisis alba.

Iota Crucis

Iota Piscis Austrini (ι Piscis Austrini) is a solitary, blue-white hued star in the southern constellation of Piscis Austrinus. It has an apparent visual magnitude of +4.35 and is around 500 light years from the Sun. This is an A-type main sequence star with a stellar classification of A0 V.

Iotroxic acid, also known as meglumine iotroxate, is a molecule used as a contrast medium during X-rays. It is specifically used during tests looking at the gallbladder and biliary tract. It is given by slow injection into a vein.Side effects are uncommon. They include vomiting, skin flushing, headache, itchiness, and low blood pressure. Rare side effects include seizures and allergic reactions. It should not be used by those who have a iodine allergy.

Iotated E (Cyrillic)

Iota Chi

Iota Sgr

Iota Herculis

Iota Scorpii

Ioudaioi

Iouliti Lymoura

Iota Cassiopeiae

Iothia is a genus of sea snails, the true limpets, marine gastropod mollusks in the family Lepetidae.

Iotichthys

Iota Chamaeleontis (ι Cha, ι Chamaeleontis) is a star in the constellation Chamaeleon. It has an apparent magnitude of about 5.3, meaning that it is just barely visible to the naked eye. Based upon parallax measurements made by the Hipparcos spacecraft, this star is around 190 light years away from the Sun. Its spectral type is F3/5 III/IV, meaning it is an F-type star, likely a subgiant; its proper motion is relatively high.

Iotacism (Greek: ιωτακισμός, iotakismos) is the process by which a number of vowels and diphthongs in Ancient Greek converged in pronunciation so they all now sound like iota ([i]) in Modern Greek. In the case of the letter eta specifically, the process is known as itacism (from the resulting pronunciation of the letter's name as [ˈita]).

Iota Normae

In formal language theory and computer science, Iota and Jot (from Greek iota ι, Hebrew yodh י, the smallest letters in those two alphabets) are languages, extremely minimalist formal systems, designed to be even simpler than other more popular alternatives, such as the lambda calculus and SKI combinator calculus. Thus, they can also be considered minimalist computer programming languages, or Turing tarpits, esoteric programming languages designed to be as small as possible but still Turing-complete. Both systems use only two symbols and involve only two operations. Both were created by professor of linguistics Chris Barker in 2001. Zot (2002) is a successor to Iota that supports input and output.

Iota Phoenicis (ι Phe) is a class A2V (white main-sequence) star in the constellation Phoenix. An Alpha² Canum Venaticorum variable, its apparent magnitude varies from 4.70 to 4.75 of a period of about 12.5 days and it is approximately 249 light years away based on parallax.It also has one companion, at a separation of 6.7" and a magnitude about 12.8.

ι Lupi, Latinised as Iota Lupi, is a solitary star in the southern constellation of Lupus. It is visible to the naked eye with an apparent visual magnitude of 3.54. Based upon an annual parallax shift of 9.65 mas as seen from Earth, it is located around 338 light years from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.23 due to interstellar dust. Relative to its neighbors, this star has a peculiar velocity of 27.4±4.9 km/s. It appears to be a member of the Scorpio-Centaurus OB association.This star has the spectrum of a B-type subgiant star with a stellar classification of B2.5 IV, which may indicate that it has used up its core supply of hydrogen and has begun to expand off the main-sequence. It is rotating rapidly with a projected rotational velocity of 370 km/s. This is giving the star an oblate shape with an equatorial bulge that is an estimated 12% larger than the polar radius. It is about 20 million years old with 6.9 times the mass of the Sun and 4 times the Sun's radius. The star radiates 2,082 times the solar luminosity from its outer atmosphere at an effective temperature of 18,605 K.

Iotroxic acid, also known as meglumine iotroxate, is a molecule used as a contrast medium during X-rays. It is specifically used during tests looking at the gallbladder and biliary tract. It is given by slow injection into a vein.Side effects are uncommon. They include vomiting, skin flushing, headache, itchiness, and low blood pressure. Rare side effects include seizures and allergic reactions. It should not be used by those who have a iodine allergy. Iotroxic acid is an iodine containing contrast media of the diionic dimer type.Iotroxic acid was first made in 1976. It is on the World Health Organization's List of Essential Medicines, the most effective and safe medicines needed in a health system. It is rarely used in the developed world due to the availability of magnetic resonance cholangiopancreatography (MRCP).

Ioukhari Veisalou

Iota and Jot

Iota Phi Theta Fraternity, Incorporated

Iota Draconis

Iota Trianguli, Latinized from ι Trianguli, is quadruple star system in constellation of Triangulum. It is approximately 290 light years from Earth.Both components of ι Trianguli are spectroscopic binaries and the brighter pair is variable. It has been given the variable star designation TZ Trianguli. The variations are due to the ellipsoidal shape of the stars as they rotate, and also it is classified as an RS Canum Venaticorum variable.

Iou

Iota Centauri

Iota Lupi

Ioulia Lipnitskaya

Iotapapillomavirus 1

Iota Centauri, Latinized from ι Centauri, is a star in the southern constellation of Centaurus. It carries the rarely applied traditional name Alhakim ("The Wise One"), dervived from the Arabic title Kentaurus al-Hakeem (قنطورس الحكيم), meaning "The Wise Centaur". Based upon parallax measurements, it lies at a distance of approximately 58.6 light-years (18.0 parsecs) from Earth.

Iota Phi Lambda

Iota Cygni

ι Sagittarii

Iota Ceti (ι Cet, ι Ceti) is the Bayer designation for a star system in the equatorial constellation of Cetus. It has the traditional name Deneb Kaitos Shemali. The name was from the Arabic word ذنب الشمالي - ðánab al-shamāliyy, meaning the northern tail of the sea monster. it is visible to the naked eye with an apparent visual magnitude of 3.562. Based upon an annual parallax shift of 11.88 mas, it lies around 275 light years from the Sun.In Chinese, 天倉 (Tiān Cāng), meaning Square Celestial Granary, refers to an asterism consisting of ι Ceti, η Ceti, θ Ceti, ζ Ceti, τ Ceti and 57 Ceti. Consequently, ι Ceti itself is known as 天倉一 (Tiān Cāng yī, English: the First Star of Square Celestial Granary.)This is an MK-standard star with a stellar classification of K1.5 III, indicating that it is an evolved K-type giant star. However, Houk and Swift (1999) list a classification of K1 II, which would indicate this is a bright giant. It is a suspected variable with a visual amplitude of around 0.05 magnitude. The star has about 2.8 times the mass of the Sun, 34 times the Sun's radius, and radiates 398 times the solar luminosity from its outer atmosphere at an effective temperature of 4,446 K.Iota Ceti forms a wide astrometric pair with a common proper motion companion, a magnitude 10.40 star at an angular separation of 106.4 arcseconds along a position angle of 191° (as of 2014). This companion may be a K-type star.

ι Volantis

* Lophiotoma cingulifera (Lamarck, 1822)

Iotam Bagration

Iota Ceti

Iota Trianguli Australis (ι Trianguli Australis) is a binary star system in the constellation Triangulum Australe. It is visible to the naked eye with a combined apparent visual magnitude of +5.27. Based upon an annual parallax shift of 25.77 mas as seen from the Earth, it is located around 127 light years from the Sun. The system appears to be moving closer to the Sun with a radial velocity of around −6 km/s. It shows itself to be composed of a yellow and a white star when seen though a 7.5 cm telescope.This is a double-lined spectroscopic binary system with an orbital period of 39.88 days and an eccentricity of 0.25. The brighter member, component A, is yellow-white hued F-type subgiant star and a Gamma Doradus type variable, pulsating by 0.12 magnitudes with a dominant period of 1.45 days. There a magnitude 9.42 visual companion, located 16.2 arcseconds away.

Ioto (Kagoshima)

Iothia fulva is a species of sea snail, a true limpet, a marine gastropod mollusk in the family Lepetidae, one of the families of true limpets.

Ioulia Sotnikova

Iota Sculptoris

Iotabrycon

Iota alpha pi

Iota Piscium

Iota Carinae

Iota Eridani

Iota Cassiopeiae (ι Cas, ι Cassiopeiae) is a star system in the constellation Cassiopeia. The system has a combined apparent magnitude of 4.53, making it visible to the naked eye. Based on its parallax, it is located about 133 light-years (41 parsecs) from Earth.

Iouga is a suggested reconstruction of the name of a Romano-British goddess known from a single fragmentary inscription on an altar-stone at York. The name appears as Ioug[...] or Iou[...] on the damaged stone, which reads:NVMINIB AVG ET DEAE IOV[...]SIVS AEDEM PRO PARTE D[...]To the numina of the Emperor(s) and to the goddess Iou[..], [..]sius (built/restored) a (half?) part of a temple.Reading the fragmentary name as Ioug[...], Roger Wright proposed the reconstructed form Iouga, which he linked with the Proto-Celtic *jugā meaning 'yoke'. However, Theresia Pantzer, reviewing the stone, suggests that what Wright had perceived as traces of a letter g was merely "damage to the stone rather than part of a letter". The goddess is otherwise unknown.

Iotated A (Ꙗ, ꙗ) is a letter of the Cyrillic script, used today only in Church Slavonic. It is unusual among early Cyrillic letters in having no direct counterpart in Glagolitic: Ⱑ (jat’) is used for both /ě/ and /ja/. Accordingly, many early Cyrillic texts (particularly those with Glagolitic antecedents) may use Ѣ for both these purposes; this practice continues into the fourteenth century, but is much more common in the South Slavonic than the East Slavonic area.

Iota Capricorni (ι Cap, ι Capricorni) is a solitary, yellow-hued star in the southern constellation of Capricornus. It can be seen with the naked eye, having an apparent visual magnitude of +4.3. Based upon an annual parallax shift of 16.58 mas as seen from the Earth, the star is located about 197 light years from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.08 due to interstellar dust.This is an evolved G-type giant star with a stellar classification of G8 III. It is classified as a BY Draconis type variable star. This is a chromospherically-active star with a longitudinal magnetic field strength of 8.3±0.6 G and an X-ray luminosity of 4.482×1030 erg s−1. The activity and photometric variation of the star allow an estimate of its rotation period as 68 days.Iota Capricorni has an estimated 2.9 times the mass of the Sun and nearly 11 times the Solar radius. It is 390 million years old and is radiating 83 times the solar luminosity from its chromosphere at an effective temperature of 5,200 K.

ι Boötis

Iotified E

Iotalamate

Iotified vowel

*Pilidium coppingeri( (E. A. Smith, 1881)

Iota Fornacis

Ioulia Kouzina

Iothalamate

Ioudaious

Iota Crateris

ι Cancri
Iota Cancri

Ioudas

Iota Beta Chi

Iota Phi Theta Fraternity, Incorporated (ΙΦΘ) is a nationally incorporated, historically African-American, collegiate fraternity whose purpose is the development and perpetuation of Scholarship, Leadership, Citizenship, Fidelity and Brotherhood among Men. It was founded on September 19, 1963, at Morgan State University (then Morgan State College) in Baltimore, Maryland. At present, it consists of over 70,000 members. There are currently over 300 undergraduate and alumni chapters, as well as colonies located in 40 U.S. states, the District of Columbia, The Bahamas, Colombia, South Korea, and Japan.The fraternity holds membership in the National Pan-Hellenic Council (NPHC), an umbrella organization comprising nine international historically African-American Greek letter sororities and fraternities, and the North-American Interfraternity Conference (NIC). The Centaur magazine is the official publication of the Iota Phi Theta Fraternity, Inc. First published as a newsletter, the Centaur has evolved into a biannual magazine.

Iotnar

Iotated

Iota Orionis (ι Orionis, abbreviated Iot Ori, ι Ori) is a multiple star system in the equatorial constellation of Orion the hunter. It is the eighth-brightest member of Orion with an apparent visual magnitude of 2.77 and also the brightest member of the asterism known as Orion's Sword. It is a member of the NGC 1980 open cluster.

Iota Horologii, Latinized from ι Horologii, is a yellow-hued star approximately 56 light-years away in the Horologium constellation. The star is classified as a G0Vp yellow dwarf (it has previously been classified as G3 and a subgiant [IV]). It has a mass and radius larger than the Sun, and is about 50% more luminous.In 1999, a planet of the star was discovered. Because the planet orbits in a near Earth orbit, Iota Horologii was ranked 69th in the list of candidates for NASA's planned Terrestrial Planet Finder mission. In 2000, a dust disc was announced around the star, but this was later determined to be an instrumental artifact.

Iota Ceti (ι Cet, ι Ceti) is the Bayer designation for a star system in the equatorial constellation of Cetus. It has the traditional name Deneb Kaitos Shemali. The name was from the Arabic word ذنب الشمالي - ðánab al-shamāliyy, meaning the northern tail of the sea monster. it is visible to the naked eye with an apparent visual magnitude of 3.562.

Iota Sagittarii (Iota Sgr, ι Sagittarii, ι Sgr) is a star in the zodiac constellation of Sagittarius. With an apparent visual magnitude of +4.118, it is bright enough to be viewed with the naked eye. Based upon an annual parallax shift of 17.94 mas as seen from Earth, this star is located 182 light years from the Sun. It is moving away from the Earth with a radial velocity of +35.8 km/s.This is a probable astrometric binary, based upon proper motion data collected during the Hipparcos mission. The visible component shows the spectrum of an evolved K-type giant or bright giant star with a stellar classification of K0 II-III. The measured angular diameter, after correction for limb darkening, is 2.32±0.02 mas. At an estimated distance of this star, this yields a physical size of about 14 times the radius of the Sun. It has 1.4 times the mass of the Sun and is radiating 87 times the Sun's luminosity from its photosphere at an effective temperature of about 4,594 K.

Ioudaismos

Iounane

Iota Sigma Pi

Iota Microscopii

Iota Lyrae

Iota Centauri, Latinized from ι Centauri, is a star in the southern constellation of Centaurus. It carries the rarely applied traditional name Alhakim ("The Wise One"), dervived from the Arabic title Kentaurus al-Hakeem (قنطورس الحكيم), meaning "The Wise Centaur". Based upon parallax measurements, it lies at a distance of approximately 58.6 light-years (18.0 parsecs) from Earth. Iota Centauri has an apparent visual magnitude of +2.73, making it easily visible to the naked eye.In Chinese, 柱 (Zhǔ), meaning Pillars, refers to an asterism consisting of ι Centauri, υ2 Centauri, υ1 Centauri, a Centauri, ψ Centauri, 4 Centauri, 3 Centauri and 1 Centauri. Consequently, ι Centauri itself is known as 柱十一 (Zhǔ shíyī, English: the Eleventh Star of Pillars.)The spectrum of ι Centauri matches a stellar classification of A2 V. It is an A-type main sequence star that is generating energy by the nuclear fusion of hydrogen in its core region. This energy is being radiated from the outer envelope of the star at an effective temperature of 8,600 K, giving the star a white hue. It has about 2.5 times the Sun's mass and is roughly 350 million years old. The abundance of elements other than hydrogen and helium, what astronomers term the metallicity, is only 35% of the abundance in the Sun. A weak magnetic field has been tentatively identified with a strength of −77 ± 30 G.This star has an excess emission of infrared indicating it is surrounded by a circumstellar disk of dust, known as a debris disk. The disk is located within an orbital radius of six Astronomical Units from the star. The dust is unusually luminous for a star this age, suggesting that some process may have recently increased the amount of debris, such as collisions between planetesimals. Alternatively, the planetesimals in this system may have unusual physical properties. As of 2011, a search for planets in this system has thus far been unsuccessful.Iota Centauri appears to belong to the stellar kinematic group known as IC 2391. This is a group of around 16 co-moving stars that most likely originated in the same molecular cloud at least 45 million years ago.

Iota Draconis (ι Draconis, abbreviated Iota Dra, ι Dra), also named Edasich, is a star in the northern circumpolar constellation of Draco. A visually unremarkable star of apparent magnitude 3.3, in 2002 it was discovered to have a planet orbiting it (designated Iota Draconis b, later named Hypatia). From parallax measurements, this star is located at a distance of about 101.2 light-years (31.0 parsecs) from the Sun.

Iota Cancri (ι Cnc, ι Cancri) is a double star in the constellation Cancer approximately 300 light years from Earth.The two stars of ι Cancri are separated by 30 arcseconds, changing only slowly. Although no orbit has been derived, the two stars show a large common proper motion and are assumed to be gravitationally related.The brighter star, ι Cancri A, is a yellow G-type bright giant with an apparent magnitude of +4.02. It is a mild barium star, thought to be formed by mass transfer of enriched material from an asymptotic giant branch star onto a less evolved companion. No such donor has been detected in the ι Cancri system, but it is assumed that there is an unseen white dwarf.The fainter of the two stars, ι Cancri B, is a white A-type main sequence dwarf with an apparent magnitude of +6.57. It is a shell star, surrounded by material expelled by its rapid rotation.

Iotica

Iouliti "Lolita" Lymoura (born March 10, 1985) is a Greek basketball player for PAOK and the Greek national team.She participated at the EuroBasket Women 2017.

Iotapa in Palaestina

Iotisis

Iota adscript

Iota Cephei (ι Cephei, ι Cep) is a solitary star in the northern constellation Cepheus. Based upon an annual parallax shift of 15.83 mas as seen from the Earth, it is located about 206 light years from the Sun. The star is visible to the naked eye with an apparent visual magnitude of 3.5.This is a K-type giant star with a stellar classification of K0 III.

Iota Gruis, Latinized from ι Gruis, is a binary star system in the southern constellation of Grus. It has an apparent visual magnitude of 3.90, which is bright enough to be seen with the naked eye at night. The distance to this system, as determined using an annual parallax shift of 17.80 mas as seen from the Earth, is about 183 light years.This is a single-lined spectroscopic binary with an orbital period of 409.6 days (1.121 years) and an eccentricity of 0.66. The yellow-hued primary component is an evolved K-type giant star with a stellar classification of K1 III. It is an X-ray emitter with a flux of 441.31×10−17 W/m2.

Iota Virginis (ι Virginis, abbreviated Iota Vir, ι Vir) is a binary star in the constellation of Virgo. Its apparent magnitude is 4.08. Based on its parallax, it is assumed to be relatively nearby, at 72.5 light-years (22.24 parsecs).Its two components are designated Iota Virginis A (also named Syrma) and B.

Iota Nu Delta

Iotam Bagration (Georgian: იოთამ ბაგრატიონი) was a Georgian royal prince (batonishvili) of the Bagrationi dynasty of House of Mukhrani branch. Iotam was son of Prince Vakhushti of Kartli.

Iota subscriptum

Iota Coronae Borealis, Latinized from ι Coronae Borealis, is a binary star system in the constellation Corona Borealis. It is visible to the naked eye with a combined apparent visual magnitude of is 4.96. Based upon an annual parallax shift of 10.46 mas as seen from the Earth, it is located about 312 light years from the Sun.This is a single-lined spectroscopic binary with an orbital period of 35.5 days and an eccentricity of 0.56. The visible member, component A, has a stellar classification of A0 IIIp(HgMnEu)s, indicating it is a chemically peculiar mercury-manganese star with narrow absorption lines. The secondary member, component B, appears to be an A-type star.

Iotapa

Iotyrris is a genus of sea snails, marine gastropod mollusks in the family Turridae, the turrids.

Iotapapillomavirus

Ioulia Lipnitskaia

Ioun

Iota chi

Iota Horologii, Latinized from ι Horologii, is a yellow-hued star approximately 56 light-years away in the Horologium constellation. The star is classified as a G0Vp yellow dwarf (it has previously been classified as G3 and a subgiant [IV]). It has a mass and radius larger than the Sun, and is about 50% more luminous.In 1999, a planet of the star was discovered.

Ioulia Timochenko

Iotyrris marquesensis is a species of sea snail, a marine gastropod mollusk in the family Turridae, the turrids.

Iotaphora admirabilis is a species of moth of the family Geometridae. It is found in south-eastern Siberia, Korea and Taiwan.

Iotapa (contemporary to Cleopatra Selene I)

Iotyrris devoizei is a species of sea snail, a marine gastropod mollusk in the family Turridae, the turrids.

Iota Geminorum (ι Gem, ι Geminorum) is a solitary fourth-magnitude star in the constellation Gemini. In the sky, it forms an isosceles triangle with Castor and Pollux, and is located less than a degree from the 5th magnitude stars 64 and 65 Geminorum. It is called by the proper name Propus, meaning "forefoot" in Latin.In Chinese, 五諸侯 (Wu Zhū Hóu), meaning Five Feudal Kings, refers to an asterism consisting of ι Geminorum, θ Geminorum, τ Geminorum, υ Geminorum and φ Geminorum.

Iota Gruis, Latinized from ι Gruis, is a binary star system in the southern constellation of Grus. It has an apparent visual magnitude of 3.90, which is bright enough to be seen with the naked eye at night. The distance to this system, as determined using an annual parallax shift of 17.80 mas as seen from the Earth, is about 183 light years.This is a single-lined spectroscopic binary with an orbital period of 409.6 days (1.121 years) and an eccentricity of 0.66.

Iou Kuroda

Iota Coronae Borealis, Latinized from ι Coronae Borealis, is a binary star system in the constellation Corona Borealis. It is visible to the naked eye with a combined apparent visual magnitude of is 4.96. Based upon an annual parallax shift of 10.46 mas as seen from the Earth, it is located about 312 light years from the Sun.This is a single-lined spectroscopic binary with an orbital period of 35.5 days and an eccentricity of 0.56.

Ioulia Pakhalina

Iota Ophiuchi (ι Oph) is a class B8V (blue main-sequence) star in the constellation Ophiuchus. Its apparent magnitude is 4.39 and it is approximately 245 light years away based on parallax.

Iota Geminorum IV

Iotifying

Iotalamic acid (also iothalamic acid in USAN) and its salts (INN Iothalamates) is an iodine-containing organic anion used as a radiocontrast agent. It is available as sodium iothalamate (Iothalamate sodium) and meglumine iothalamate (Iothalmate meglumine). It can be administered intravenously or intravesically (into the urinary bladder).Radioactive formulation is also available as sodium iothalamate I-125 Injection (GLOFIL-125).

Iota Island, Bermuda

Iota subscript

Iou Kuroda (黒田硫黄, Kuroda Iō, [kɯɾoda i.oː], born January 5, 1971) is the pen name of a Japanese manga artist.

Iouktas

Iotrolan (trade name Isovist) is a radiocontrast agent, a substance used to improve the visibility of body structures on images obtained by X-ray techniques. It is particularly used to image spaces surrounding the central nervous system, such as the ventricles, after injection into the cerebrospinal fluid. It can also be used to image joint spaces and in endoscopic retrograde cholangiopancreatography (ERCP).Chemically, the substance is a dimer of triiodinated isophthalic acid derivatives.

Iota Beta Chi (ΙΒΧ) is a Canadian national sorority. There are two active chapters in Atlantic Canada to date; one in Halifax, Nova Scotia, and the other in Fredericton, New Brunswick.

Iota Microscopii (ι Mic) is a class F1IV (yellow-white subgiant) star in the constellation Microscopium. Its apparent magnitude is 5.11 and it is approximately 116 light years away based on parallax.It has one companion, first observed in 1932, with a separation of 4.3" and a visual magnitude of 15.5.

Iota Eridani (ι Eri) is a solitary star in the constellation Eridanus. It is visible to the naked eye with an apparent magnitude of 4.11. With an annual parallax shift of 0.02165 arcseconds, it lies at an estimated distance of about 151 light years.This is a evolved red clump giant star with a stellar classification of K0 III. The measured angular diameter, after correcting for limb darkening, is 2.18±0.02 mas. At an estimated distance of the star, this yields a physical size of around 11 times the radius of the Sun. It has 1.42 times the mass of the Sun and radiates 57.5 times the solar luminosity from its outer atmosphere at an effective temperature of 4,683 K. It is around four billion years old.

Ioujima, Nagasaki

Iota Draconis b

Iota Virginis

Ioulia Shapiro

Ioudaios

Iota Librae

Ioudaike

Iota Sweethearts

*Tectura (Pilidium) coppingeri( E. A. Smith, 1881)

Iotapa (daughter of Artavasdes I)

Iotated Yat

Iouji-mae Station

Iota Persei

Iota Horologii b

Iota Leporis (ι Leporis) is a triple star system in the southern constellation of Lepus. It is visible to the naked eye as a point source of blue-white light with an apparent visual magnitude of 4.45. Based upon an annual parallax shift of 14.07 mas as measured from Earth, the system is located roughly 232 light years from the Sun.The primary, designated component A, is a B-type main-sequence star with a stellar classification of B7.5 Vn, where the 'n' suffix indicates "nebulous" absorption lines caused by rotation. It is about 94 million years old and has a high rate of spin with a projected rotational velocity of 185 km/s. With an estimated 3.4 times the mass of the Sun, it is radiating 153 times the Sun's luminosity from its photosphere at an effective temperature of around 13,781 K.There is a close companion that is a source of X-ray emission. Most likely this star has at least 1.05 times the mass of the Sun. The third component, AM Leporis, is a BY Draconis variable of apparent magnitude 9.92, and spectral type G8Ve at an angular separation of 12.7".

Iota phi theta

Ioudaikou

ι Centauri

Iotified Yat

The iota subscript is a diacritic mark in the Greek alphabet shaped like a small vertical stroke or miniature iota ⟨ι⟩ placed below the letter. It can occur with the vowel letters eta ⟨η⟩, omega ⟨ω⟩, and alpha ⟨α⟩. It represents the former presence of an [i] offglide after the vowel, forming a so‐called "long diphthong".

violet

Ioudaikē archaiologia

ι Crateris

The iota subscript is a diacritic mark in the Greek alphabet shaped like a small vertical stroke or miniature iota ⟨ι⟩ placed below the letter. It can occur with the vowel letters eta ⟨η⟩, omega ⟨ω⟩, and alpha ⟨α⟩. It represents the former presence of an [i] offglide after the vowel, forming a so‐called "long diphthong". Such diphthongs (i.e., ηι, ωι, ᾱι)—phonologically distinct from the corresponding normal or "short" diphthongs (i.e., ει, οι, ᾰι )—were a feature of ancient Greek in the classical era. The offglide was lost in pronunciation during the Hellenistic period with the result that from approximately the 1st century BC onwards the former diphthongs were no longer distinguished from the simple long vowels η, ω, ᾱ respectively. During the Roman and Byzantine eras, the iota, now mute, was sometimes still written as a normal letter but was often simply left out. The iota subscript was invented by Byzantine philologists in the 12th century AD as an editorial symbol marking the places where such spelling variation occurred.The alternative practice, of writing the mute iota as a full-sized letter ⟨ι⟩, is known as iota adscript.

Iota Phoenicis

Iota Cancri (ι Cnc, ι Cancri) is a double star in the constellation Cancer approximately 300 light years from Earth.The two stars of ι Cancri are separated by 30 arcseconds, changing only slowly. Although no orbit has been derived, the two stars show a large common proper motion and are assumed to be gravitationally related.The brighter star, ι Cancri A, is a yellow G-type bright giant with an apparent magnitude of +4.02.

Ioudaios (Ancient Greek: Ἰουδαῖος; pl. Ἰουδαῖοι Ioudaioi) is an Ancient Greek ethnonym used in classical and biblical literature which commonly translates to "Jew" or "Judean".The choice of translation is the subject of frequent scholarly debate, given its central importance to passages in the Bible (both the Hebrew Bible and the New Testament) as well as works of other writers such as Josephus and Philo. Translating it as Jews is seen to imply connotations as to the religious beliefs of the people, whereas translating it as Judeans confines the identity within the geopolitical boundaries of Judea.A related translation debate refers to the terms ἰουδαΐζειν (verb), literally translated as "Judaizing" (compare Judaizers), and Ἰουδαϊσμός (noun), controversially translated as Judaism or Judeanism.

Iouik, also spelled Iwik, is a coastal town in western Mauritania.

Iota Leonis, Latinized from ι Leonis, is a triple star system in the constellation Leo. The system is fairly close to the Sun, at only 79 light-years (24.2 parsecs) away, based on its parallax. The system has a combined apparent magnitude of 4.00 making it faintly visible to the naked eye. It is moving closer to the Sun with a radial velocity of −10 km/s.Iota Leonis has a spectral type of F3 IV, matching that of an F-type subgiant star.

ι Microscopii

Iouiya

Iota Orionis (ι Orionis, abbreviated Iot Ori, ι Ori) is a multiple star system in the equatorial constellation of Orion the hunter. It is the eighth-brightest member of Orion with an apparent visual magnitude of 2.77 and also the brightest member of the asterism known as Orion's Sword. It is a member of the NGC 1980 open cluster. From parallax measurements, it is located at a distance of roughly 2,300 light-years (710 parsecs) from the Sun.The system has three components designated Iota Orionis A, B and C. Iota Orionis A is itself a massive spectroscopic binary, with components Iota Orionis Aa (also named Hatysa) and Ab.

Iothia coppingeri

Iota Phi Lambda Sorority, Inc.