quarta-feira, 15 de junho de 2016

Sírius, a mais bela dentre as belas, vem despedindo-se de nossos olhares, ao cair da noite

Olá!

Qual estrela é a mais bela dos céus estrelados?
Sírius, com toda a certeza todos dirão.

Sirius, em função de sua proximidade, 
é conhecida como a estrela mais brilhante
- mesmo que esteja a 8 anos-luz de distância de nós.  

A bem da verdade, 
muitíssimas outras estrelas são mais brilhantes do que Sirius 
porém situando-se extremamente mais distanciadas 
e portando parecendo bem mais pálidas 
do que esta estrela tão próxima a nós.

Sírius vem despedindo-se de nossos olhares,
ao cair da noite,
mergulhando mais e mais cedo
para esconder-se atrás do horizonte oeste.

Porém, mais algumas semanas à frente,
Caro Leitor,
esta belíssima estrela-alpha Canis Majoris, Sirius,
estará reaparecendo no horizonte leste,
na madrugada sonolenta,
ainda antes da chegada do Sol,
mais ao finalzinho do mês de julho.

Sirius não é uma estrela somente
e sim um sistema binário,
sendo que a outra estrela é denominada de Sirius B
enquanto Sirius é também conhecida como Sirius A.

Nesta Postagem, Caro Leitor,
encontre informações sobre Sirius A e Sirius B
e ainda também informações sobre as demais estrelas
que podemos observar na direção da constelação do Cão Maior,
Canis Major,
bem como uma estrela hípergigante, VY Canis Majoris




Stellarium

Stellarium

Stellarium




Sirius.  Alpha Canis Majoris.  Estrela Dupla
Ascensão Reta 06h 44,2m - Declinação -16o 42’
Magnitude visual - 1,58 e 7,6  -  Distância 8 anos-luz
Distância entre estrelas 11”,16

O Ardente, nome latino da estrela mais brilhante, segundo os antigos gregos. 
Uma estrela binária, branco brilhante e amarelo, situada na boca do Cão Maior.  
De Seirios, possivelmente do deus egípcio Osíris. 
Entre os egípcios também era considerada como Thoth e Sothis.  
Os chinêses conheciam como Tseen Lang, o Lobo dos Céus, 
e diziam que quando estava muitíssimo brilhante é porque os ladrões iriam atacar.

Sirius B, a outra componente, 
foi a primeira estrela branca anã a ser descoberta.

Sirius, em função de sua proximidade, 
é conhecida como a estrela mais brilhante.  


6a. Edição do Atlas Celeste
de autoria de Ronaldo Rogério de Freitas Mourão,
Editora Vozes, Petrópolis, ano de 1986


File:Sirius A and B Hubble photo.jpg

Author
NASA, ESA
Credit: H. Bond (STScI) and M. Barstow (University of Leicester)

The image of Sirius A and Sirius B taken by the 
Hubble Space Telescope
The white dwarf can be seen to the lower left.[64] 
Thediffraction spikes and concentric rings areinstrumental effects.





A bem da verdade, 
muitíssimas outras estrelas são mais brilhantes do que Sirius 
porém situando-se extremamente mais distanciadas 
e portando parecendo bem mais pálidas 
do que esta estrela tão próxima a nós.


Sírio (Sirius, α CMa, α Canis Majoris, Alpha Canis Majoris) é a estrela mais brilhante no céu noturno, com uma magnitude aparente de −1,46, localizada na constelaçãode Canis Major. Pode ser vista a partir de qualquer ponto na Terra, sendo que, no Hemisfério Norte faz parte do Hexágono do Inverno.
Dista 2,6 parsecs (ou 8,57 anos-luz) da Terra, sendo por isso uma das estrelas mais próximas do nosso planeta. A sua estrela vizinha mais próxima é Procyon, à distância de 1,61 pc ou 5,24 anos-luz, com um espectro de tipo A0 ou A1 e uma massa cerca de 2,4 vezes maior que a massa do Sol.
A melhor época do ano para observação situa-se em meados do mês de janeiro, quando atinge o meridiano à meia-noite.
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Etimologia

O termo Sirius deriva do latim sīrius e do grego σείριος (seirios, "brilhante").
Sendo a principal estrela da constelação do “Cão Maior”, é muitas vezes apelidada de “Estrela do Cão” ou “Estrela Canina”.
Também é conhecida pelo nome latino “Canicula” (“pequeno cachorro”) e como الشعرى aš-ši’rā, em árabe, donde deriva o nome alternativo “Ascherre”.
................................................................................................


Sírio A / B
Posição de Sírio (Sirius) na constelação de Cão Maior.
Dados observacionais (J2000)
ConstelaçãoCanis Major
Asc. reta06h 45m 08.9173s
Declinação-16° 42′ 58″
Magnitude aparente-1,46
Características
Tipo espectralA1V
Cor (U-B)0,01
Cor (B-V)-0,05
Astrometria
Velocidade radial-7,6 km/s
Mov. próprio (AR)RA: −546,05
Paralaxe379,21 ± 1,58
Distância8,6 ± 0,04 anos-luz
2,64 ± 0,01 pc
Magnitude absoluta1,42
Detalhes
Massa2,02 M
Raio1,711 R
Gravidade superficial(log g) 4,33 (A)/8,57 (B)
Luminosidade25,4 L
Temperatura9 940 K
Metalicidade[Fe/H] =0,50
Rotação-16 km/s
Idade2–3 × 108 anos
Outras denominações
Sistema: Sirius, Estrela do Cão, Aschere, Canícula, Al Shira, Sothis, Mrgavyadha, Lubdhaka, Tenrōsei, α Canis Majoris (α CMa), 9 Canis Majoris (9 CMa), HD 48915, HR2491, BD −16°1591, GCTP 1577.00 A/B, GJ244 A/B, LHS 219, ADS 5423, LTT 2638, HIP 32349.
B: EGGR 49, WD 0642-166
Sirius
Canis major constellation map.png
https://pt.wikipedia.org/wiki/Sirius

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Sistema binário

Em 1844Friedrich Wilhelm Bessel deduzira que Sirius era na verdade um sistema binário e em 1862 Alvan Graham Clark identificara a estrela companheira, apelidando-a de Sirius B ou, carinhosamente, “o cachorrinho”, sendo que as duas estrelas orbitam entre si separadas por 20 unidades astronômicas aproximadamente. A estrela visível a olho nu é actualmente referida como Sirius A.
Em 1915 astrônomos do Observatório de Monte Wilson determinaram que Sirius B era uma anã branca, a primeira a ser descoberta. Curiosamente, isso significa que Sirius B terá tido originalmente uma massa muito superior à de Sirius A.





.......................................

AB Binary Star System
After analyzing the motions of Sirius from 1833 to 1844, Friedrich Wilhelm Bessel (1784-1846) concluded that it had an unseen companion. Sirius B itself was not actually observed until January 31, 1862 by Alvan Graham Clark (1832-1897), who was testing a new 18-inch telescope built for Dearborn Observatory by the famous company founded by his father (Alvan Clark) and later run by his brother and himself. Clark was soon honored with the Lalande prize of the French Academy for his discovery. Star B's peculiar high temperature, small size, and great density, however, were not established until 1925 by Walter Sydney Adams (1876-1956).


McDonald Observatory -- larger image



Sirius is a binary star system.

Sirius is composed of a main-sequence star and a white dwarf stellar remnant. They form a close binary, Alpha Canis Majoris A and B, that is separated "on average" by only about 20 times the distance from the Earth to the Sun -- 19.8 astronomical units (AUs) of an orbital semi-major axis -- which is about the same as the distance between Uranus and our Sun ("Sol"). The companion star, is so dim that it cannot be perceived with the naked eye.
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Caro leitor, encontre mais e mais informações interessantes sobre Sirius AB, acessando
http://www.solstation.com/stars/sirius2.htm






http://hubblesite.org/newscenter/archive/releases/2005/36/image/a/format/web_print/

ABOUT THIS IMAGE:

This Hubble Space Telescope image shows Sirius A, the brightest star in our nighttime sky, along with its faint, tiny stellar companion, Sirius B. Astronomers overexposed the image of Sirius A [at center] so that the dim Sirius B [tiny dot at lower left] could be seen. The cross-shaped diffraction spikes and concentric rings around Sirius A, and the small ring around Sirius B, are artifacts produced within the telescope's imaging system. The two stars revolve around each other every 50 years. Sirius A, only 8.6 light-years from Earth, is the fifth closest star system known.
Sirius B, a white dwarf, is very faint because of its tiny size, only 7,500 miles in diameter. White dwarfs are the leftover remnants of stars similar to the sun. They have exhausted their nuclear fuel sources and have collapsed down to a very small size. Sirius B is about 10,000 times fainter than Sirius A. ..........................................................................................................................................
This image was taken Oct. 15, 2003, with Hubble's Wide Field Planetary Camera 2. Based on detailed measurements of the position of Sirius B in this image, astronomers were then able to point the STIS instrument exactly on the white dwarf and make the measurements to determine its gravitational redshift and mass.
Object Name: Sirius A and Sirius B
Image Type: Astronomical
Credit: NASA, H.E. Bond and E. Nelan (Space Telescope Science Institute, Baltimore, Md.); M. Barstow and M. Burleigh (University of Leicester, U.K.); and J.B. Holberg (University of Arizona)

http://hubblesite.org/newscenter/archive/releases/2005/36/image/a/





Hail, mighty Sirius, monarch of the suns!
May we in this poor planet speak with thee?
Mrs. Sigourney's The Stars.

α, Binary, ‑1.43 and 8.5, brilliant white and yellow.

Sirius, the Dog-star, often written Syrius even as late as Flamsteed's and Father Hell's day, has generally been derived from σείριος, sparkling or scorching, which first appeared with Hesiod as a title for this star, although also applied to the sun, and by Abychos to all the stars. Various early Greek authors used it for our Sirius, perhaps generally as an adjective, for we read in Eratosthenes:
Such stars astronomers call σειρίους on account of the tremulous motion of their light;
so that it would seem that the word, in its forms σείρσείρος, and σείριος, — Suidas used all three for both sun and star, — originally was employed to indicate any bright and sparkling heavenly object, but in the course of time became a proper name for this brightest of all the stars. Lamb, however, thought it of Phoenician origin, signifying the Chief One, and originally in that country a title for the sun; Jacob Bryant, the mythologist, said that it was from the Egyptians' Cahen Sihor; but Brown considers it a transcription from their well-known Hesiri, the GreekOsiris; while Dupuis distinctly asserted that it was from the Celtic Syr.
Plutarch called it Προόπτης, the Leader, which well agrees with its character and is an almost exact translation of its Euphratean, Persian, Phoenician, and Vedic titles; but ΚύωνΚύων σείριοςΚύων ἀστήρΣείριος ἀστήρΣείριον ἄστρον, or simply το ἄστρον, were its names in early Greek astronomy and poetry. Προκύων, better known for the Lesser Dog and its lucida, also was applied to Sirius by Galen as preceding the other stars in the constellation.
Homer alluded to it in the Iliad as Ὀπωρινός, the Star of Autumn;1 but the season intended was the last days of July, all of August, and part of September — the latter part of summer. Lord Derby translated this celebrated passage:
A fiery light
There flash'd, like autumn's star, that brightest shines
When newly risen from his ocean bath;
p121while later on in the poem Homer compares Achilles, when viewed by Priam, to
th' autumnal star, whose brilliant ray
Shines eminent amid the depth of night,
Whom men the dog-star of Orion call.
The Roman farmers sacrificed to it a fawn-colored dog at their three festivals when, in May, the sun began to approach Sirius. These, instituted 238 B.C., were the Robigalia, to secure the propitious influence of their goddess Robigo in averting rust and mildew from their fields; and theFloralia and Vinalia, to ensure the maturity of their blooming flowers, fruits and grapes.
Among the Latins it naturally shared the constellation's titles, probably originated them; and occasionally was even Canicula; indeed, as late as 1420 the Palladium of Husbandry urged certain farm-work to be done "Er the caniculere, the hounde ascende"; and, more than a century later, Eden, in the Historie of the Vyage to Moscovie and Cathay, wrote: "Serius is otherwise called Canicula, this is the dogge, of whom the canicular days have theyr name."c
It has been asserted that Ovid and Vergil referred to Sirius in their Latrator Anubis, representing a jackal, or dog-headed Egyptian divinity, guardian of the visible horizon and of the solstices, transferred to Rome as goddess of the chase; but it is very doubtful whether they had in mind either star or constellation.
Its well-known name, Al Shiʽrā, or Al Siʽrā, extended as al Abūr al Yamaniyyah, much resembles the Egyptian, Persian, Phoenician, Greek, and Roman equivalents, and, Ideler thought, may have had common origin with them from some one ancient, source: possibly the Sanskrit Sūrya, the Shining One, — the Sun. The ʽAbur, or Passage, refers to the myth of Canopus' flight to the South; and the adjective to the same, or perhaps to the southerly position of the star towards Yemen, in distinction from that of Al Ghumaisā᾽ in the Lesser Dog, seen towards Shām, — Syria, — in the North. From these geographical names originated the Arabic adjectives Yamaniyyah and Shamāliyyah, Southern and Northern; although the former literally signifies On the Right-hand Side, i.e. to an observer facing eastward towards Mecca.
In Chrysococca's Tables the title is Σιαὴρ Ιαμανὴ; and Doctor C. Edward Sachau's translation of Al Bīrūnī's Chronology renders it Sirius Jemenicus. Riccioli had Halabor, which the 1515 Almagest applied to the constellation; and Chilmead, GabbarEcber, and Habor; while Shaari lobur, another p122queerly corrupted form, is found in Eber's Egyptian Princess. In the Alfonsine Tables the original is changed to Asceher and Aschere Aliemini; while Bayer gives plain Aschere and Elscheere for the star, with others similar for both star and constellation. Scera is cited by Grotius for the star, and Sceara for the whole, derived from an old lexicon; and Alsere; but he traced all to Σείριος.
In modern Arabia it is Suhail, the general designation for bright stars.
The late Finnish poet Zakris Topelius accounted for the exceptional magnitude of Sirius by the fact that the lovers Zulamith the Bold and Salami the Fair, after a thousand years of separation and toil while building their bridge, the Milky Way, upon meeting at its completion,
Straight rushed into each other's arms
And melted into one;
So they became the brightest star
In heaven's high arch that dwelt —
Great Sirius, the mighty Sun
Beneath Orion's belt.
The native Australians knew it as their Eagle, a constellation by itself; while the Hervey Islanders, calling it Mere, associated it in their folklore with Aldebaran and the Pleiades.
Sharing the Sanskrit titles for the whole, it was the Deer-slayer and the Hunter, while the Vedas also have for it Tishiya or TishigaTistrija,Tishtrya, the Tistar, or Chieftain'sStar. And this we find too in Persia; as also Sira. The later Persian and Pahlavi have Tir, the Arrow. Edkins, however, considers Sirius, or Procyon, to be Vanand, and Arcturus, Tistar.
Hewitt sees in Sirius the Sivānam, or Dog, of the Rig Veda awakening the Ribhus, the gods of mid-air, who "thus calls them to their office of rain sending," a very different office from that assigned to this star in Rome. Yet these gods, philologically, had a Roman connection, for Professor Friedrich Maximilian Mueller, writing the word Arbhu, associates it with the Latin Orpheus. Hewitt also says that in the earliest Hindu mythology Sirius was Sukra, the Rain-god, before Indra was thus known; and that in the Avesta it marked one of the Four Quarters of the Heavens.
Although the identification of Euphratean stellar titles is by no means settled, especially and singularly so as to this great star, yet various authorities have found for it names more or less probable.
Berlin and Brown think it conclusively proved that it was Kak-shisha, the Dog that Leads, and "a Star of the South"; while Kak-shidi is Sayce's transliteration of the original signifying the Creator of Prosperity, a character which the Persians also assigned to it; and it may have been the p123Akkadian Du-shisha, the Director — in Assyrian Mes-ri-e. Epping and Strassmaier have Kak-ban as a late Chaldaean title, which Brown rendersKal‑bu, the Dog, "exactly the name for Sirius we should expect to find"; Jensen has Kakkab lik-ku, the Star of the Dog, revived in Homer's κύων; and it perhaps was the Assyrian Kal-bu Sa-mas, the Dog of the Sun; and the Akkadian Mul-lik-ud, the Star Dog of the Sun. Jensen also givesKakkab kasti, the Bow Star, although this may be doubtful; and Brown has, from the Assyrian, Su-ku-du, the Restless, Impetuous, Blazing, well characterizing the marked scintillation and color changes in its light. Hewitt cites an Akkadian title Tis-khu.
Its risings and settings were regularly tabulated in Chaldaea about 300 B.C., and Oppert is reported to have recently said that the Babylonian astronomers could not have known certain astronomical periods, which as a matter of fact they did know, if they had not observed Sirius from the island of Zylos in the Persian Gulf on Thursday, the 29th of April, 11542 B.C.!º
It is the only star known to us with absolute certitude in the Egyptian records — its hieroglyph, a dog, often appearing on the monuments and temple walls throughout the Nile country. Its worship, chiefly in the north, perhaps, did not commence till about 3285 B.C., when its heliacal rising at the summer solstice marked Egypt's New Year and the beginning of the inundation, although precession has now carried this rising to the 10th of August. At that early date, according to Lockyer, Sirius had replaced γ Draconis as an orientation point, especially at Thebes, and notably in the great temple of Queen Hatshepsu, known to-day as Al Dēr al Bahārī, the Arabs' translation of the modern Copts' Convent of the North. Here it was symbolized, under the title of Isis Hathor, by the form of a cow with disc and horns appearing from behind the western hills. With the same title, and styled Her Majesty of Denderah, it is seen in the small temple of Isis, erected 700 B.C., which was oriented toward it; as well as on the walls of the great Memnonium, the Ramesseum, of Al Ḳurneh at Thebes, probably erected about the same time that this star's worship began. Lockyer thinks that he has found seven temples oriented to the rising of Sirius. It is also represented on the walls of the recently discovered step-temple of Saḳḳara, dating from about 2700 B.C., and supposed to have been erected in its honor.
Great prominence is given to it on the square zodiac of Denderah, where it is figured as a cow recumbent in a boat with head surmounted by a star; and again, immediately following, as the goddess Sothis, accompanied by the goddess Anget, with two urns from which water is flowing, emblematic p124of the inundation at the rising of the star. But in the earlier temple service of Denderah it was Isis Sothis, at Philae Isis Sati, or Satit, and, for a long time in Egypt's mythology, the resting-place of the soul of that goddess, and thus a favorable star. Plutarch made distinct reference to this [de Iside 359D]; although it should be noted that the word Isis at times also indicated anything luminous to the eastward heralding sunrise. Later it was Osiris, brother and husband of Isis, but this word also was applied to any celestial body becoming invisible by its setting. Thus its titles noticeably changed in the long period of Egypt's history.
As Thoth, and the most prominent stellar object in the worship of that country, — its heliacal rising was in the month of Thoth, — it was in some way associated with the similarly prominent sacred ibis, also a symbol of Isis and Thoth, for, in various forms, the bird and star appear together on Nile monuments, temple walls, and zodiacs.
Sirius was worshiped, too, as Sihor, the Nile Star, and, even more commonly, as Sothi and Sothis, its popular Graeco-Egyptian name, theBrightly Radiating One, the Fair Star of the Waters; but in the vernacular was SeptSepetSopet, and SopditSed,2 and Sot, — the Σήθ of Vettius Valens.
Upon this star was laid the foundation of the Canicular, Sothic, or Sothiac Period named after it, which has excited the attention and puzzled the minds of historians, antiquarians, and chronologists. Lockyer has an admirable discussion of this in his Dawn of Astronomy.
Sir Edwin Arnold writes of it in his Egyptian Princess:
And even when the Star of Kneph has brought the summer round,
And the Nile rises fast and full along the thirsty ground;
for the Egyptians always attributed to the Dog-star the beneficial influence of the inundation that began at the summer solstice; indeed, some have said that the Aethiopian Nile took from Sirius its name Siris, although others consider the reverse to be the case. Minsheu, who dwells much on this, ends thus: "Some thinke that the Dog-starre is called Sirius, because at the time the Dogge-starre reigneth, Nilus also overfloweth as though the water were led by that Starre." Indeed, it has been fancifully asserted that its canine title originated in Egypt, "because of its supposed watchful care over the interests of the husbandman; its rising giving him notice of the approaching overflow of the Nile."
Caesius cited for it Solechin as from that country, signifying the Starry Dog, and derived from the Egypto-Greek word Σολεκήν.
p125Perhaps it is the ancient importance of this Dog on the Nile that has given the popular name, the Egyptian X, to the figure formed by the stars Procyon and Betelgeuze, Naos and Phaet, with Sirius at the vertices of the two triangles and the centre of the letter. On our maps Sirius marks the nose of the Dog.
The Phoenicians are said to have known it as Hannabeah, the Barker.
The astronomers of China do not seem to have made as much of Sirius as did those of other countries, but it is occasionally mentioned, with other stars in Canis Major, as Lang Hoo; and Reeves quoted for it Tseen Lang, the Heavenly Wolf. Their astrologers said that when unusually bright it portended attacks from thieves.
Some have called it the Mazzārōth of the Book of Job; others the Ḣaṣīl of the Hebrews; but this people also knew it as Sihor, its Egyptian name, and Ideler thinks that the adoration of the Sɛērīm, or "Devils" of the Authorized Version of our Bible, the "He Goats" of the Revision, which, as we see in Leviticus xvii.7, was specially prohibited to the Jews, may have had reference to Sirius and Procyon, the Two Sirii or Shiʽrayān, that must have been well known to them in the land of their long bondage as worshiped by their taskmasters.
The culmination of this star at midnight was celebrated in the great temple of Ceres at Eleusis, probably at the initiation of the Eleusinian mysteries; and the Ceans of the Cyclades predicted from its appearance at its heliacal rising whether the ensuing year would be healthy or the reverse. In Arabia, too, it was an object of veneration, especially by the tribe of Kais, and probably by that of Kodhā'a, although Muḥammad expressly forbade this star-worship on the part of his followers. Yet he himself gave much honor to some "star" in the heavens that may have been this.
In early astrology and poetry there is no end to the evil influences that were attributed to Sirius.
Homer wrote, in Lord Derby's translation,
The brightest he, but sign to mortal man
Of evil augury.
Pope's very liberal version of the same lines, —
Terrific glory! for his burning breath
Taints the red air with fevers, plagues and death, —
seems to have been taken from the Shepheard's Kalendar for July:
The rampant Lyon hunts he fast with dogge of noysome breath
Whose baleful barking brings in hast pyne, plagues and dreerye death.
Spenser, however, was equally a borrower, for we find in the Aeneid:
p126The dogstar, that burning constellation, when he brings drought and diseases on sickly mortals, rises and saddens the sky with inauspicious light;
and in the 4th Georgic:
Jam rapidus torrens sitientes Sirius Indos
Ardebat coelo,
rendered by Owen Meredith in his Paraphrase on Vergil's Bees of Aristaeus:
Swift Sirius, scorching thirsty Ind,
Was hot in heaven.
Hesiod advised his country neighbors, "When Sirius parches head and knees, and the body is dried up by reason of heat, then sit in the shade and drink," — advice universally followed, even till now, although with but little thought of Sirius. Hippocrates made much, in his Epidemics andAphorisms, of this star's power over the weather, and the consequent physical effect upon mankind, some of his theories being current in Italy even during the last century; while the result of all physic depended upon the sign of the zodiac in which the sun chanced to be. Manilius wrote of Sirius:
from his nature flow
The most afflicting powers that rule below.
But these expressions as to the hateful character of the Dog-star may have been induced in part from the evil reputation of the dog in the East.
Its heliacal rising, 400 years before our era, corresponded with the sun's entrance into the constellation Leo, that marked the hottest time of the year, and this observation, originally from Egypt, taken on trust by the Romans, who were not proficient observers, and without consideration as to its correctness for their age and country, gave rise to their dies caniculariae, the dog days, and the association of the celestial Dog and Lion with the heat of midsummer. The time and duration of these days, although not generally agreed upon in ancient times, any more than in modern, were commonly considered as beginning on the 3d of July and ending on the 11th of August, for such were the time and period of the unhealthy season of Italy, and all attributed to Sirius. The Greeks, however, generally assigned fifty days to the influence of the Dog-star. Yet even then some took a more correct view of the matter, for Geminos wrote:
It is generally believed that Sirius produces the heat of the dog days; but this is an error, for the star merely marks a season of the year when the sun's heat is the greatest.
But he was an astronomer.
p127The idea prevailed, however, even with the sensible Dante in his "great scourge of days canicular"; while Milton, in Lycidas, designated it as "the swart star." And the notion holds good with many even to the present time. This character doubtless is indicated on the Farnese globe, where the Dog's head is surrounded with sun-rays.
But Pliny took a kinder view of this star, as in the "xii. chapyture of the xi. booke of his naturall hystorie," [XI.XII.30] on the origin of honey:
This coometh from the ayer at the rysynge of certeyne starres, and especially at the rysynge of Sirius, and not before the rysynge of Vergiliae (which are the seven starres cauled Pleiades) in the sprynge of the day;
although he seems to be in doubt whether "this bee the swette of heaven, or as it were a certeyne spettyl of the starres." This idea is first seen in Aristotle's History of Animals. So, too, in late astrology wealth and renown were the happy lot of all born under this and its companion Dog. Our modern Willis wrote in his Scholar of Thebet ben Khorat:
Mild Sirius tinct with dewy violet,
Set like a flower upon the breast of Eve.
When in opposition Sirius was supposed to produce the cold of winter.
It has been in all history the brightest star in the heavens, thought worthy by Pliny of a place by itself among the constellations, and even seen in broad sunshine with the naked eye by Bond at Cambridge, Massachusetts, and by others at midday with very slight optical aid; but its color is believed by many to have changed from red to its present white. This question recently has been discussed, by See in the affirmative and Schiaparelli in the negative, at a length not allowing repetition here, the weight of argument, however, seeming to be against the admission of any change of color in historic times.
Aratos' term ποικίλος, applied to the Dog, is equally appropriate to Sirius now in the sense of many-colored or changeful, and is an admirable characterization, as one realizes when watching this magnificent object coming up from the horizon on a winter evening. Tennyson, who is always correct as well as poetical in his astronomical allusions, says in The Princess:
the fiery Sirius alters hue
And bickers into red and emerald;
this, of course, being largely due to its marked scintillation; and Arago gave Barāḳish as an Arabic designation for Sirius, meaning Of a Thousand p128Colors; and said that as many as thirty changes of hue in a second had been observed in it.3
Sirius, notwithstanding its brilliancy, is by no means the nearest star to our system, although it is among the nearest; only two or three others having, so far as is yet known, a smaller distance. Investigations up to the present time show a parallax of 0ʺ.39, indicating a distance of 8.3 light years, nearly twice that of α Centauri.
Some are of the opinion that the apparent magnitude of Sirius is partly due to the whiteness of its tint and its greater intrinsic brilliancy; and that the red stars, Aldebaran, Betelgeuze, and others, would appear much brighter than now if of the same color as Sirius; rays of red light affecting the retina of the eye more slowly than those of other colors. The modern scale of magnitudes that makes this star ‑1.43, — about 9½ times as bright as the standard 1st-magnitude star Altair (α Aquilae), — would make the sun ‑25.4, or 7000 million times as bright as Sirius; but, taking distance into account, we find that Sirius is really forty times brighter than the sun.
Its spectrum, as type of the Sirian in distinction from the Solar, gives name to one of the four general divisions of stellar spectra instituted by Secchi from his observations in 1863‑67; these two divisions including nearly 11/12 of the observed stars. Of these about one half are Sirian of a
brilliantly white colour, sometimes inclining towards a steely blue. The sign manual of hydrogen is stamped upon them with extraordinary intensity
by broad, dark shaded lines which form a regular series.
It is found by Vogel to be approaching our system at the rate of nearly ten miles a second, and, since Rome was built, has changed its position by somewhat more than the angular diameter of the moon.
It culminates on the 11th of February.
The celebrated Kant thought that Sirius was the central sun of the Milky Way; and, eighteen centuries before him, the poet Manilius said that it was "a distant sun to illuminate remote bodies," showing that even at that early day some had knowledge of the true character and office of the stars.
Certain peculiarities in the motion of Sirius led Bessel in 1844, after ten years of observation, to the belief that it had an obscure companion with which it was in revolution; and computations by Peters and Auwers led Safford to locating the position of the satellite, where it was found as p129predicted on the 31st of January, 1862, by the late Alvan Clark,4 at Cambridgeport, Mass., while testing the 18½-inch glass now at the Dearborn Observatory. It proved to be a yellowish star, estimated as of the 8½ magnitude, but difficult to be seen because of the brilliancy of Sirius, and then 10ʺ away; this diminishing to 5ʺ in 1889; and last seen and measured by Burnham at the Lick Observatory before its final disappearance in April, 1890. Its reappearance was observed from the same place in the autumn of 1896 at a distance of 3ʺ.7, with a position angle of 195°. It has a period of 51½ years, and an orbit whose diameter is between those of Uranus and Neptune; its mass being one third that of Sirius and equal to that of our sun, although its light is but 1/10000 its principal, soº that it may be supposed to be approaching non-luminous solidity, — one of Bessel's "dark stars."
It is remarkable that Voltaire in his Micromegas of 1752, an imitation of Gulliver's Travels, followed Dean Swift's so‑called prophetic discovery of the two moons of Mars by a similar discovery of an immense satellite of Sirius, the home of his hero. Swift, however, owed his inspiration to Kepler, who more than a century previously wrote to Galileo:
I am so far from disbelieving in the existence of the four circumjovial planets, that I long for a telescope to anticipate you, if possible, in discovering two round Mars (as the proportion seems to me to require), six or eight round Saturn, and perhaps one each round Mercury and Venus.
Other stars are shown by the largest glasses in the immediate vicinity of Sirius, two additional having very recently been discovered by Barnard at the Yerkes Observatory.
The text is in the public domain.

http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Canis_Major*.html






Stellarium


OUTRAS ESTRELAS
ACOMPANHANDO SÍRIUS
NA DIREÇÃO DA CONSTELAÇÃO
CANIS MAJOR,
O CÃO MAIOR:

Mirzam ou Musim - Beta Canis Majoris
É uma estrela que aparece ainda antes de Sirius, a mais brilhante dos céus, 
e por isso foi  chamada pelos egípcios de Aquela que Anuncia.  
O Precursor Daquele que Atravessa a Via Láctea, segundo a uronografia árabe. 
A Mediadora, variante do vocábulo árabe Mirzam ou Mirzar.


Phurud ou Farud  - Zeta Canis Majoris
A Única Brilhante, proveniente do árabe Al Furud, ou talvez por transcrição errônea de Al Kurud, o Macaco,
 referindo-se às pequenas estrelas  que envolvem a constelação de Columba.

Wezen - Delta Canis Majoris
O Peso, oriundo do nome árabe Al Wazn, ou seja, o peso, 
para designar que a es trela parece se levantar com dificuldade no horizonte.


Adhara - Epsilon Canis Majoris
Ascensão Reta 06h 57,8m - Declinação - 28o 57’
Magnitude visual 1,63 - Distância 680 anos-luz
As Virgens. Denominação árabe para designar, originalmente, o grupo de estrelas Omicron, Delta, Epsilon e Eta Canis Majoris.


Pi Canis Majoris - Estrela Dupla
 AR 06h53m  Dec -20o.04
M 4,6 e 9,5  Distância entre estrelas 12”,00

Aludra - Eta Canis Majoris
As Virgens, nome que, segundo a uranografia árabe, designa o asterismo formado por quatro estrelas.


Alubra - Eta Canis Majoris
A Pata, denominação árabe que representa a pata dianteira esquerda do Cão Maior.


Muliphen - Gamma Canis Majoris
A Pata Estirada, oriundo do árabe Al Muhlifain, que também é usado para designar Gama, Zeta e Lambda de Argos 
e Alpha e Beta Columbae.


6a. Edição do Atlas Celeste
de autoria de Ronaldo Rogério de Freitas Mourão,
Editora Vozes, Petrópolis, ano de 1986




 
VY Canis Majoris (VY CMa) is a red hypergiant in the constellation Canis Major. It is one of the largest known stars by radius and also one of the most luminous of its type. It is approximately 1,420 ± 120 solar radii[8] (equal to 6.6 astronomical units, thus a diameter about 1,975,000,000 kilometres (1.227×109 mi)), and about 1.2 kiloparsecs (3,900 light-years) distant from Earth. VY CMa is a single star categorized as a semiregular variable and has an estimated period of 2,000 days. It has an average density of 5 to 10 mg/m3. If placed at the center of the Solar System, VY Canis Majoris's surface would extend beyond the orbit of Jupiter, although there is still considerable variation in estimates of the radius, with some making it larger than the orbit of Saturn
 A size comparison between the Sun and UY Canis Majoris.
"Sun and VY Canis Majoris" by User:Mysid - Self-made in Inkscape.. Licensed under Public Domain via Wikimedia Commons - http://commons.wikimedia.org/wiki/File:Sun_and_VY_Canis_Majoris.svg#/media/File:Sun_and_VY_Canis_Majoris.svg



Size comparison between the Sun and VY Canis Majoris
Observation dataEpoch J2000      Equinox J2000
07h 22m 58.32877s[1]
−25° 46′ 03.2355″[1]
6.5 to 9.6[2]
7.9607[3]
Characteristics
M3[4]-M5e Ia[5]
B−V color index
2.24[4]
49 ± 10[4] km/s
RA: 9.84[4] mas/yr
Dec.: 0.75[4] mas/yr
Parallax (π)
0.83 ± 0.1[7] mas
~3,840 ly
(1,170
[8] [9] pc)
Details
17 ± 8[8] M
1420 ± 120[8] R
~270,000[8] L
Surface gravity (log g)
-0.6[8] cgs
~3,490[8] K


File:Rho Cassiopeiae Sol VY Canis Majoris.png

Algumas estrelas monstruosas comparadas com nosso Sol e a órbita de Júpiter e Neptuno. Da esquerda para a direita: The Pistol Star, Rho Cassiopeiae, Betelgeuse, e VY Canis Majoris.


VEJA OS VÍDEOS:
O Planeta Terra comparado a uma das maiores estrelas do Universo

VY Canis Majoris

Escala de corpos celestes - Da Lua à VY Canis MajorisVY Canis Majoris



Canis Major
http://www.aradergalleries.com/detail.php?id=3644
Johann Bayer — Canis Major


COM UM ABRAÇO ESTRELADO,
Janine Milward