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Mula (nakshatra)
Mūla ('root'; Devanagari मूल/मूळ, , , ) is the 19th ''nakshatra'' or 'lunar mansion' in Jyotisha and corresponds to the stars: λ Sco, υ Sco, ε Sco, μ1 Sco, θ Sco, κ Sco, ι1 Sco, and ζ1 Sco. The symbol of Mula is a bunch of roots tied together (reticulated roots) or an 'elephant goad' (ankusha) and the Deity associated with it is Niriti, the god of dissolution and destruction. The Lord of Mula is Ketu KETU (1120 AM) is a commercial radio station licensed to Catoosa, Oklahoma, and serving the Tulsa metropolitan area. The station broadcasts a Spanish adult contemporary radio format and is owned by Antonio Perez, through licensee Radio Las Amer ... (south lunar as a node). The Ascendant/Lagna in Mula indicates a person who has a passionate desire to get to the truth and is good at investigation and research. They are direct, ardent and truthful and are shrewd and ambitious, but they can feel trapped and bound by circumstances and so feel resentmen ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Devanagari
Devanagari ( ; in script: , , ) is an Indic script used in the Indian subcontinent. It is a left-to-right abugida (a type of segmental Writing systems#Segmental systems: alphabets, writing system), based on the ancient ''Brāhmī script, Brāhmī'' script. It is one of the official scripts of India, official scripts of India and Nepal. It was developed in, and was in regular use by, the 8th century CE. It had achieved its modern form by 1000 CE. The Devanāgarī script, composed of 48 primary characters, including 14 vowels and 34 consonants, is the fourth most widely List of writing systems by adoption, adopted writing system in the world, being used for over 120 languages, the most popular of which is Hindi (). The orthography of this script reflects the pronunciation of the language. Unlike the Latin alphabet, the script has no concept of letter case, meaning the script is a unicase, unicameral alphabet. It is written from left to right, has a strong preference for symmetri ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Nakshatra
Nakshatra () is the term for Lunar mansion in Hindu astrology and Buddhist astrology. A nakshatra is one of 27 (sometimes also 28) sectors along the ecliptic. Their names are related to a prominent star or asterisms in or near the respective sectors. In essence (in Western astronomical terms), a nakshatra simply is a constellation. Every nakshatra is divided into four ''padas'' ( "steps"). The starting point for the nakshatras according to the ''Vedas'' is "Krittika" (it has been argued, because the Pleiades may have started the year at the time the ''Vedas'' were compiled, presumably at the vernal equinox), but, in more recent compilations, the start of the nakshatras list is the point on the ecliptic directly opposite the star Spica, called ''Chitrā'' in Sanskrit. This translates to Ashwinī, a part of the modern constellation of Aries. These compilations, therefore, may have been compiled during the centuries when the sun was passing through Aries at the time of the ver ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Lambda Scorpii
Lambda Scorpii is a triple star system and the second-brightest object in the constellation of Scorpius. It is formally named Shaula; ''Lambda Scorpii'' is its Bayer designation, which is Latinised from λ Scorpii and abbreviated Lambda Sco or λ Sco. With an apparent visual magnitude of 1.62, it is one of the brightest stars in the night sky. Nomenclature ''λ Scorpii'' (Latinised to ''Lambda Scorpii'') is the star system's Bayer designation. It bore the traditional name ''Shaula'', which comes from the Arabic الشولاء ''al-šawlā´'' meaning 'the raised ail, as it is found in the tail of Scorpius, the scorpion. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN, which included ''Shaula'' for the star λ Scorpii Aa. In Indian Astronomy it is called MulA ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Upsilon Scorpii
Upsilon Scorpii (υ Scorpii, abbreviated Upsilon Sco, υ Sco), formally named Lesath , is a star located in the "stinger" of the southern zodiac constellation of Scorpius, the scorpion. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 580 light-years from the Sun. In the night sky it lies near the 1.6 magnitude star Lambda Scorpii, and the two form an optical pair that is sometimes called the "Cat's Eyes". Nomenclature ''υ Scorpii'' ( Latinised to ''Upsilon Scorpii'') is the star's Bayer designation. It bore the traditional name ''Lesath'' (alternatively spelled ''Leschath'', ''Lesuth''), from the Arabic ''las'a'' "pass (or bite) of a poisonous animal"; but this is a miscorrection by Scaliger (a European astronomer who knew Arabic) for earlier "Alascha", which came from Arabic ''al laţkha'' "the foggy patch", referring to the nearby open cluster M7. In 2016, the International Astronomical Union organized a Working Group on ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Epsilon Scorpii
Epsilon Scorpii (ε Scorpii, abbreviated Eps Sco, ε Sco), formally named Larawag , is a star in the southern zodiac constellation of Scorpius. It has an apparent visual magnitude of +2.3, making it the fifth-brightest member of the constellation. Parallax measurements made during the Hipparcos mission provide an estimated distance to this star of around from the Sun. Epsilon Scorpii has a stellar classification of K1 III, which indicates it has exhausted the supply of hydrogen at its core and evolved into a giant star. The interferometry-measured angular diameter of this star, after correcting for limb darkening, is , which, at its estimated distance, equates to a physical radius of nearly 12 times the radius of the Sun. Presently it is generating energy through the nuclear fusion of helium at its core, which, considering the star's composition, places it along an evolutionary branch termed the red clump. The star's outer atmosphere has an effective temperature ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Mu1 Scorpii
Mu1 Scorpii (μ1 Scorpii, abbreviated Mu1 Sco, μ1 Sco) is a binary star system in the southern zodiac constellation of Scorpius. The combined apparent visual magnitude of the pair is about magnitude 3, making it one of the brighter members of Scorpius. Based upon parallax measurements, the distance of this system from the Sun is roughly 500 light-years (150 parsecs). This system is a member of the Scorpius–Centaurus association, the nearest OB association of co-moving stars to the Sun. The primary (Mu1 Scorpii Aa) is formally named Xamidimura , from the Khoekhoe 'the (two) eyes of the lion'. Properties Mu1 Scorpii is an eclipsing binary of the Beta Lyrae type. Discovered to be a spectroscopic binary by Solon Irving Bailey in 1896, it was only the third such eclipsing pair to be discovered. This is a semidetached binary system where the secondary is close to filling its Roche lobe, or it may even be overflowing. The two stars revolve each other alon ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Theta Scorpii
Theta Scorpii (θ Scorpii, abbreviated Theta Sco, θ Sco) is a binary star in the southern zodiac constellation of Scorpius. The apparent visual magnitude of this star is +1.87, making it readily visible to the naked eye and one of the brightest stars in the night sky. It is sufficiently near that the distance can be measured directly using the parallax technique and such measurements obtained during the ''Hipparcos'' mission yield an estimate of approximately from the Sun. The two components are designated θ Scorpii A (officially named Sargas , the traditional name for the system) and B. Nomenclature ''θ Scorpii'' ( Latinised to ''Theta Scorpii'') is the system's Bayer designation. The designations of the two components as ''Theta Scorpii A'' and ''B'' derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). It bore the traditional name ''Sargas'', of Sumerian o ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Kappa Scorpii
Kappa Scorpii, Latinisation of names, Latinized from κ Scorpii, is a binary star system in the southern constellation of Scorpius. With an apparent visual magnitude of 2.4, this star system is readily visible to the naked eye. Parallax measurements place it at an estimated distance of roughly from the Earth. Properties This is a spectroscopic binary, which is a type of binary star system in which the two stars are so close together that they have not been individually resolved with a telescope. The pair orbit each other with a orbital period, period of about 195 days and an orbital eccentricity, eccentricity of about 0.5. The combined stellar spectrum, spectrum of this pair matches a star with a stellar classification of B1.5 III. The 'III' luminosity class indicates the presence of a giant star that has exhausted the supply of hydrogen at its core and is in a late stellar evolution, evolutionary stage. The primary component of the pair, κ Sco A, is a variable s ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Iota1 Scorpii
Iota1 Scorpii, Latinisation of names, Latinized from ι1 Scorpii, is a star in the southern constellation of Scorpius. With an apparent visual magnitude of 3.03, this star can be seen with the naked eye. It is sometimes called by the proper name Apollyon. Parallax measurements place it at a distance of roughly from Earth, with a 9% margin of error. At the estimated distance, the apparent magnitude is diminished by 0.66magnitudes due to intervening gas and dust between Earth and the star. This star has a stellar classification of F2 Ia, with the 'Ia' luminosity class indicating this is a supergiant more luminous than typical supergiants. It has about 12 times the solar mass, Sun's mass and is 35,000 times more luminous. The limb darkening, limb-darkened angular diameter of Iota1 Scorpii is estimated at . At the estimated distance, this corresponds to a physical radius of . The effective temperature of the photosphere is 6,910 or 7,103 K, which gives it a yellow- ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Zeta1 Scorpii
Zeta1 Scorpii (Zeta1 Sco, ζ1 Scorpii, ζ1 Sco) is a B-type hypergiant star in the constellation of Scorpius. It has an apparent visual magnitude which varies between 4.66 and 4.86. It is a member of the Scorpius OB1 association, and potentially of the open star cluster NGC 6231, also known as the "Northern jewel box" cluster. ζ1 Scorpii is a luminous blue variable according to its luminosity and spectral appearance, yet is has not shown the characteristic types of variability, hence is classified as a dormant LBV. Around 36 times as massive as the Sun, it is one of the most luminous stars known in the Galaxy, with an estimated bolometric luminosity between 850,000 and 1.3 million times that of the Sun and a radius 103 to 126 times that of the Sun. The stellar wind from this supergiant is expelling matter from the star at the rate of per year, or roughly the equivalent to the Sun's mass every 640,000 years. ζ1 Scorpii forms a naked eye d ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Ankusha
The elephant goad, bullhook, or ankusha is a tool employed by mahout in the elephant handling, handling and training of elephants. The pointed tip of an elephant goad or a bullhook could be used to stab the elephant's head if the elephant charged nearby people, risking injury or death to the rider and bystanders. The elephant goad consists of a hook (usually bronze or steel) which is attached to a handle, ending in a tapered end. A relief at Sanchi and a fresco at the Ajanta Caves depict a three-person crew on the war elephant, the driver with an elephant goad, what appears to be a noble warrior behind the driver and another attendant on the posterior of the elephant.Nossov, Konstantin & Dennis, Peter (2008). ''War Elephants''. illustrated by Peter Dennis. Edition: illustrated. Osprey Publishing.(accessed: Monday April 13, 2009), p.18 Nossov and Dennis (2008: p. 19) report that two perfectly preserved elephant goads were recovered from an archaeological site at Taxila and are d ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
