The nebula itself is of relatively low surface brightness compared to the central star,[65] and is undersized for the primary's mass for reasons not yet fully understood. Gas from the surface of the donor star is transferred to the accreting star, and the transfer of mass dominates the system’s evolution. It was the northern pole star around the year 12,000 BC and will be again around the year 13,727. It represents the lyre, a musical instrument with strings used in antiquity and later times. Vega was the pole star in the year 12,000 BCE, and will again become the pole star around 14,000 CE. [49] Another evolved star is EP Lyrae, a faint RV Tauri variable and an "extreme example" of a post-AGB star. RR Lyrae is the brightest star in this class, with an apparent magnitude ranging from 7.06 to 8.12. Vega is easy to find in the night sky because it is bright and also because it is part of a familiar summer asterism, the Summer Triangle, which it forms with the stars Altair in the constellation Aquila and Deneb in Cygnus. The primary star has the stellar classification of B7II – it is a blue-white bright giant. Véga est sur l'alignement qui part de la Grande Ourse, suivant la diagonale SO-NE de la « casserole ». Originally thought to be possibly due to the presence of an Earth-like planet, it is now accepted that the irregularities are due to a large starspot. Voir plus d'idées sur le thème Constellation, La lyre, Nebuleuse. abundance of elements other than hydrogen and helium. [72], In orbit around the orange subgiant star HD 177830 is one of the earliest exoplanets to be detected. Mu Lyrae is a white subgiant star belonging to the spectral class A3IVn. [53], One of the most peculiar systems in Lyra is MV Lyrae, a nova-like star consisting of a red dwarf and a white dwarf. It has an apparent magnitude of 4.323 and is approximately 238 light years distant from the solar system. cette. RR Lyrae est le prototype d'une catégorie d'étoiles variables pulsantes nommées variables de type RR Lyrae. Altaïr fait partie de la constellation de l’Aigle, visible l’été et au début de l’automne. Without Orpheus and his music, the Argonauts would not have been able to make it past the Sirens, whose song enticed sailors to come to them, which usually resulted in sailors crashing their ships into the islands on which the Sirens lived. NGC 6791, image: NASA, ESA, Digitized Sky Survey, and L. Bedin (STScI). La constellation est d'ailleurs proche du Cygne et de l'Aigle. La Lyre était l’une des 48 constellations identifiées par Ptolémée. The nebula was formed when a shell of ionized gas was expelled by a red giant star that was in the process of becoming a white dwarf. It has between 30 and 40 Jupiter masses. Certains ont même connecté avec les Pléiades (par exemple, Ovide, qui a mentionné que les sept cordes de la Lyre égalé le nombre des Pléiades). [9] The constellation's boundaries, as set by Belgian astronomer Eugène Delporte in 1930, are defined by a 17-sided polygon. The system is 26.5 light years distant from the Sun. The cluster is about 84 light years across. Cet alignement passe par le cœur du Dragon et par sa tête, pour venir toucher Véga, puis plus loin Altaïr de l'Aigle. [11], German cartographer Johann Bayer used the Greek letters alpha through nu to label the most prominent stars in the constellation. Line: 478 Il étaitsur le mont Pangée, attendant le lever du Soleil, pour êtrele premier à lui rendre hommage (Eratosthène),lorsq… On dit que, comme il honorait singulièrement Apollon,en qui il voyait le plus grand des dieux, et qu'il ne redait aucun honneura Dionysos / Bacchus,a qui il devait une partie de sa gloire, ce dieu l'en punit. It appears prominently in the northern sky during the Northern Hemisphere's summer, and the whole constellation is visible for at least part of the year to observers north of latitude 42°S. Véga est l’étoile la plus brillante de la constellation de la Lyre. [41] Also nearby is the faint HP Lyrae, a post-asymptotic giant branch (AGB) star that shows variability. [42], In the extreme east is RR Lyrae, the prototype of the large class of variables known as RR Lyrae variables, which are pulsating variables similar to Cepheids, but are evolved population II stars of spectral types A and F. Such stars are usually not found in a galaxy's thin disk, but rather in the galactic halo. La constellation du Taureau se reconnait bien avec sa forme en A renversé, où le petit triangle représente la tête de l’animal, et les jambes de la lettre sont ses cornes. In April 2013, it was announced that of the five planets orbiting Kepler-62, at least two—Kepler-62e and Kepler-62f—are within the boundaries of the habitable zone of that star, where scientists think liquid water could exist, and are both candidates for being a solid, rocky, earth-like planet. [34][35] It may be a representative of a very brief phase in which the system is transitioning into a contact binary. It was discovered by Charles Messier on January 19, 1779. Lyra contains two Messier objects – Messier 56 (M56, NGC 6779) and Messier 57 (M57, NGC 6720, Ring Nebula) – and has nine stars with known planets. Several million years ago, it collided with a smaller galaxy, which created a region filled with young, hot, blue stars. Detected from a transit of its parent star, the planet has around 3/4 the mass of Jupiter, yet orbits its parent star in only three days. In telescopes, the nebula appears as a visible ring with a green tinge; it is slightly elliptical because its three-dimensional shape is a torus or cylinder seen from a slight angle. The area corresponding to Lyra was seen by the Arabs as a vulture or an eagle carrying a lyre, either enclosed in its wings, or in its beak. Delta-1 Lyrae is a binary star system with an orbital period of about 88 days. La constellation de la Lyre est l'une des 88 constellations de l'hémisphère Nord. D'un point de vue astrophysique, cette géante bleue (type spectral A0) de magnitude 3,2 est intrinsèquement 40 fois plus brillante que Véga, elle-même — rappelons-le — 50 fois plus brillante que le Soleil. Vous y verrez se lever une étoile bien brillante, la plus brillante du ciel d’été. Some of its characteristics are similar to those of recurring novae. Once there, his song deeply moved Hades and his wife Persephone and they agreed to return Eurydice to the world of the living on one condition: Orpheus should walk in front of her and not look back until they both had reached the upper world. The stars of Epsilon-2 Lyrae are separated by 2.3 arc seconds and have magnitudes of 5.1 and 5.5. It may have at least one planet the size of Jupiter in its orbit. The name Sulafat is derived from the Arabic al-sulḥafāt, which means “the turtle,” and Jugum comes from the Latin word iugum, meaning “yoke.”. They are old, metal-poor stars with an average absolute magnitude of 0.75, and only 40 to 50 times more luminous than the Sun. Certaines de ces étoiles principales sont : Certains des objets du ciel profond qui ont été découverts dans Lyra incluent : Messier 56, The Ring Nebula, NGC 6791, NGC 6745, IC 1296. Publié le 11 mars 2003 (mis à jour le 8 août 2015). [62] It was discovered in 1779 by Antoine Darquier, 15 years after Charles Messier discovered the Dumbbell Nebula. The star serves as a prototype of an entire class of stars, known as the RR Lyrae variables. cette see, en début de soirée, se lève vers l'est l'étoile véga, l'astre le plus brillant de la lyre. Cet instrument à cordes aurait été façonné par Hermès à partir de la carapace d’une tortue qu’il avait trouvée devant sa grotte du mont Cyllène, en Arcadie. The Ring Nebula – Messier 57 (M57, NGC 6720). C'est la position la plus extrême que le pôle puisse avoir par rapport à sa position actuelle, le lieu des pôles est un cercle dont le diamètre est sensiblement le segment Véga - α Ursae Minoris. Alors que le monde s'effondre, il y a des choses qui ne changent pas. It represents the lyre, a musical instrument with strings used in antiquity and later times. [44], Another evolved star is the naked-eye variable XY Lyrae, a red bright giant[38] just north of Vega that varies between 6th and 7th magnitudes over a period of 120 days. It has an apparent magnitude of 4.30 and is approximately 740 light years distant. Ovid tells a rather different story, saying that women, in retribution for Orpheus's rejection of marriage offers, ganged up and threw stones and spears. The superficially normal B stars ζ Draconis, η Lyrae, 8 Cygni and 22 Cygni", "Photometric UBV period study of eight AP stars", "Superhumps in Cataclysmic Binaries. With an apparent magnitude of 0.03, it is also the fifth brightest star in the night sky, after Sirius in Canis Major, Canopus in Carina, Arcturus in Boötes, and Alpha Centauri A in Centaurus constellation. [43] The easternmost star designated by Flamsteed, 19 Lyrae, is also a small-amplitude variable, an Alpha2 Canum Venaticorum variable with a period of just over one day. Sous la forme d'un vautour, cette constellation s'est raccrochée à la légende d'Hercule qui, pour son 6 e travail, tua les oiseaux du lac Stymphale. symbolisant l'instrument de musique offert par hermès à orphée, la lyre est également appelée la « carapace de tortue » ou « l'aigle aux ailes fermées » (al nasr al waki, à l'opposé de « l'aigle volant » : al nasr al taïr, notre constellation de l'aigle actuelle). W varies between 7th and 12th magnitudes over approximately 200 days,[48] while S, slightly fainter, is a silicate carbon star, likely of the J-type. It belongs to the spectral class B9 III. [6] Lyra was known as Urcuchillay by the Incas and was worshipped as an animal deity. The star is believed to be 75 million years old. The smaller galaxy is believed to have lost most of its interstellar medium to the larger one in the collision. Deux autres étoiles de la constellation portent un nom : Aladfar (η Lyr) et Alathfar (μ Lyr). Orpheus was known for his ability to charm even stones with his music, for his attempts to save his wife Eurydice from the underworld, and for being the harpist and companion of Jason and the Argonauts. Orpheus was the son of the Thracian King Oeagrus and the muse Calliope. The Ring Nebula, Messier 57, is a famous planetary nebula in Lyra constellation, located south of the bright star Vega, about 40% of the distance from Beta to Gamma Lyrae. Epsilon Lyrae has a fifth component, discovered in 1985. Both components are main-sequence stars, the primary being late F-type and the secondary late G-type. Sous la forme d'un vautour, cette constellation s'est raccrochée à la légende d'Hercule qui, pour son 6 e travail, tua les oiseaux du lac Stymphale. It has an apparent magnitude of 8.3 and is approximately 32,900 light years distant from the solar system. The brightest star in the constellation is Vega (Alpha Lyrae), a main-sequence star of spectral type A0Va. [9][n 2] Its main asterism consists of six stars,[n 3] and 73 stars in total are brighter than magnitude 6.5. [58] The true nova HR Lyrae flared in 1919 to a maximum magnitude of 6.5, over 9.5 magnitudes higher than in quiescence. [47] W and S Lyrae are two of the many Mira variables in Lyra. La constellation est d'ailleurs proche du Cygne et de l'Aigle. It has an apparent magnitude of 3.52 and is approximately 960 light years distant from Earth. The Double Double, Epsilon Lyrae, image: Robert Mura. At the time of its discovery, it was one of the hottest known exoplanets, in orbit around the F-type main-sequence star WASP-3. C'est de cette appellation arabe que vient le nom de son étoile la plus lumineuse : Vega. Gliese 747AB is a nearby star system composed of two red dwarf stars of the spectral types M3 and M5. Kappa Lyrae is an orange giant with the stellar classification of K2III. It is a relatively fast rotator, with a projected rotational velocity of 71-72 km/s. cette see, en début de soirée, se lève vers l'est l'étoile véga, l'astre le plus brillant de la lyre. RR Lyrae’s variability was first discovered by the Scottish astronomer Williamina Fleming in 1901. Lyra constellation was often depicted as a vulture or an eagle carrying Orpheus’ lyre in its wings or beak, and called Aquila Cadens or Vultur Cadens, which means “the falling eagle” or “falling vulture.”. Dans la mythologie, Lyra est la lyre du musicien talentueux Orphée. It was first catalogued by the astronomer Ptolemy in the 2nd century. As is evolved into a giant, it transferred most of its mass to the other star, as the two are in close orbit. [50], Rather close to Earth at a distance of only 16 parsecs (52 ly) is Gliese 758. Ancien Scout puis Pionnier? As soon as he reached it, he turned around, but Eurydice was not quite up there yet and she disappeared from his sight, for good this time. Zeta forms a wide binary star visible in binoculars, consisting of an Am star and an F-type subgiant. La Voie lactée sert de toile de fond à cette constellation. It was discovered by the French astronomer Antoine Darquier de Pellepoix in January 1779, and Charles Messier discovered it independently later the same month, and included it in his catalogue as the 57th object. The constellation is associated with the myth of the Greek musician and poet Orpheus. The gods felt pity for him and advised him to travel to the underworld and try to retrieve Eurydice. Such stars serve as standard candles, and thus are a reliable way to calculate distances to the globular clusters in which they reside. It can easily be seen in binoculars. The two orbit each other with a period of 12.9414 days and periodically eclipse each other. Orpheus took their advice. Function: view, File: /home/ah0ejbmyowku/public_html/index.php The star belongs to the spectral class A0V, which makes it a white dwarf. Orpheus's music was said to be so great that even inanimate objects such as trees, streams, and rocks could be charmed. Attention cependant : la méthode pour repérer Véga n’est valable que les mois d’été ! It is believed to be around 8 billion years old. [59], M57, also known as the "Ring Nebula" and NGC 6720,[61] has a diameter of one light-year and is at a distance of 2,000 light-years from Earth. As a result, their apparent magnitude varies. [85] Kepler-37 is another star with an exoplanet discovered by Kepler; the planet is the smallest known extrasolar planet known as of February 2013. Les deux premières composantes sont facilement séparables avec des jumelles et leurs belles couleurs contrastées bleues et rouges sont visibles. Vega is the brightest star in the Lyra constellation. Elle fait partie de la famille de constellation Hercules. [30] RR Lyrae itself varies between magnitudes 7 and 8 while exhibiting the Blazhko effect. Vega is located at the vertex of the triangle, and easy to find because the constellation Cygnus, the Swan, is easily recognizable in the sky. L'anneau est en fait un nuage de gaz éjecté par une étoile centrale. Liens [modifier | … Line: 315 [55] Its nature is still not fully understood. Function: _error_handler, File: /home/ah0ejbmyowku/public_html/application/views/user/popup_harry_book.php NGC 6745 – A large spiral galaxy, with its nucleus still intact, peers at the smaller passing galaxy (nearly out of the field of view at lower right), while a bright blue beak and bright whitish-blue top feathers show the distinct path taken during the smaller galaxy’s journey. The larger galaxy, NGC 6745A, is believed to have been a spiral galaxy before the collision, but now appears peculiar as a result of the encounter. [21], Vega also forms one vertex of a much smaller triangle, along with Epsilon and Zeta Lyrae. The brightest stars in it are 13th magnitude, and it contains about a dozen variables. The star is similar to the Sun. It has an apparent magnitude of 9.5 and is approximately 13,30 light years distant from the solar system. The Beta Lyrae system has a variable luminosity, ranging from 3.4 to 4.3 magnitudes. [57] Of the same type is V344 Lyrae, notable for an extremely short period between superoutbursts coupled with one of the highest amplitudes for such a period. L’Aigle représente Aphrodite métamorphosée en cet animal lorsqu’elle poursuivait le cygne qui fécondera Léda. It is classified as a variable star. The stars have apparent magnitudes of 4.7 and 6.2 and an orbital period of about 1,200 years. The variability was first discovered by the British astronomer John Goodricke in 1784. His lyre was carried to heaven by the Muses, who also collected the fragments of his body and buried them below Mount Olympus. The exoplanets are 1.6 and 1.4 times the diameter of Earth respectively, with their star Kepler-62 at a distance of 1,200 light-years. Tout en haut, tu verras une étoile très brillante. [22] Epsilon is a more famous wide binary that can even be separated by the naked eye under good conditions. The B7II star, now the less massive component, was once the more massive component in the system. Also known as 13 Lyrae, it is a 4th-magnitude red giant semiregular variable that varies by several tenths of a magnitude. à…, Découvre l'un des tout premiers moyens de s'orienter sur la planète ! While fleeing from an attack by Aristaeus, she stepped on a snake that bit her, killing her. DM Lyrae is a dwarf nova, a cataclysmic variable star composed of a close binary system in which one of the stars is a white dwarf that accretes matter from the companion star. Caractéristique des cieux d’été, le Triangle de l’été est formé par trois étoiles facilement repérables, car très brillantes : Véga, Altaïr et Deneb. [83] The Kepler-20 system contains five known planets; three of them are only slightly smaller than Neptune,[84] and two while the other two are some of the first Earth-sized exoplanets to be discovered. Lyra constellation lies in the northern sky. [14], The brightest star not included in the asterism and the westernmost cataloged by Bayer or Flamsteed is Kappa Lyrae, a typical red giant[38] around 73 parsecs distant. [56] Another outbursting star is AY Lyrae, an SU Ursae Majoris-type dwarf nova that has undergone several superoutbursts. Il passe par α du Capricorne et les deux « pieds » du capricorne ; et pour les observateurs situés suffisamment au sud, cet alignement se prolonge jusqu'à Al Na'ir (α Gruis). La constellation se reconnaît à sa forme : Véga est une étoile très brillante, qui se reconnaît par son association avec les deux étoiles plus faibles (mag 3) β et γ Lyr, l'ensemble évoquant un club de golf. The cluster was discovered by the German astronomer Friedrich August Theodor Winnecke in 1853. 22 mai 2017 - Explorez le tableau « CONSTELLATION DE LA LYRE » de Matthieu Labrosse, auquel 200 utilisateurs de Pinterest sont abonnés. Line: 192 It is unique in that it is the only known Cepheid in the Milky Way to undergo periodic phase and amplitude changes, analogous to the Blazhko effect in RR Lyrae stars. Function: view, File: /home/ah0ejbmyowku/public_html/application/controllers/Main.php The most recent one, in 1996, was a very long and bright one, indicating that the star is a variable of the SU Ursae Majoris type, one that has super-outbursts in addition to normal outbursts. La constellation est d'ailleurs proche du Cygne et de l'Aigle. one of the brightest stars in the night sky, "Elemental abundance analyses with DAO spectrograms", 10.1002/1521-3994(200207)323:2<87::AID-ASNA87>3.0.CO;2-P, "Variable Star Type Designations in the VSX", American Association of Variable Star Observers, "Spectroscopy and eclipse-mapping of the mass-exchanging binary star V361 LYR", "Late-type members of young stellar kinematic groups - I. It has an apparent magnitude of 3.261 and is approximately 620 light years distant from the Sun. The Persian Hafiz called it the Lyre of Zurah. outre la très brillante véga, cette constellation renferme aussi m ou une étoile double/double. L’une d’elles, Véga, est la cinquième étoile la plus brillante du firmament. en été, elle est presque au zénith cette see, en début de soirée, se lève vers l'est l'étoile véga, l'astre le plus brillant de la lyre. It contains three age groups of stars: 4 billion year-old white dwarfs, 6 billion year-old white dwarfs and 8 billion year-old normal stars. [45] Also just visible to the naked eye is the peculiar classical Cepheid V473 Lyrae. However, he forgot that they both had to arrive to the upper world before he could turn. OSR nomme des étoiles pour des individus du monde entier depuis le début du millénaire, et est désormais le service d’enregistrement d’étoile numéro un dans le monde. The central star, V477 Lyrae, is an eclipsing post-common-envelope binary, consisting of a white dwarf primary and an oversized secondary component due to recent accretion. Around 190 parsecs distant,[14] it has been referred to as a "superficially normal" star. Elle est assez proche du Système solaire puisqu'elle n'est distante que de 25 années-lumière. [27] The plane of the orbit is aligned with Earth and the system thus shows eclipses, dropping nearly a full magnitude from its 3rd-magnitude baseline every 13 days,[28] although its period is increasing by around 19 seconds per year. High relative velocities cause ram pressures at the surface of contact between the interacting interstellar clouds. When he was young, god Apollo gave him a golden lyre and taught him to play it, and his mother taught him to write verses. c'est de cette appellation arabe que vient le nom de son étoile. [63] Astronomers have determined that it is between 6,000 and 8,000 years old;[62] it is approximately one light-year in diameter. It is a suspected variable star and a rapid rotator, with a projected rotational velocity of 274 km/s at the equator. The sunlike primary star has a brown dwarf companion, the coldest to have been imaged around a sunlike star in thermal light when it was discovered in 2009. [64] The outer part of the nebula appears red in photographs because of emission from ionized hydrogen. © LaToileScoute, Association loi 1901, 2001 - 2020 | Site réalisé avec SPIP | Politique de confidentialité | Nous contacter The star is approximately 350 light years distant from the solar system. The Ring Nebula belongs to the class of planetary nebulae known as bipolar nebulae. [16] Vega was the first star other than the Sun to be photographed,[17] as well as the first to have a clear spectrum recorded, showing absorption lines for the first time. Attention cependant : la méthode pour repérer Véga n’est valable que les mois d’été ! outre la très brillante véga, cette constellation renferme aussi m ou une étoile double/double. Credit: A. Fujii. Droit de reproduction libre sous certaines conditions Elle fait partie de la famille de constellation Hercules. It is 6,500 times more luminous than the Sun and has a radius 200 times solar. It is one of the oldest and most metal-rich clusters known in the Milky Way. de très nombreux exemples de phrases traduites contenant "constellation de la lyre" dictionnaire anglaisfrançais et moteur de recherche de traductions anglaises. cette, véga, l'étoile la plus brillante du ciel d'été, est facile à repérer en début de soirée. It was first catalogued by the astronomer Ptolemy in the 2nd century. Line: 479 si vous regardez en direction du nordest en début de soirée, vous verrez facilement véga, l'étoile principale de Accueil > Magazine > Ces scouts changent le monde, Accueil > Déjà culte > Récits de camps scouts, Accueil > Déjà culte > Éclaireurs israélites, Accueil > Déjà culte > Éclaireurs unionistes EEUDF, Accueil > Déjà culte > Éclaireuses Éclaireurs de France, Accueil > Déjà culte > Éclaireuses et Éclaireurs de la Nature, Accueil > Déjà culte > Fédération Éclaireurs FEE, Accueil > Déjà culte > Guides et Scouts d’Europe, Accueil > Déjà culte > Inter-mouvements scouts, Accueil > Déjà culte > Scouts et Guides de France, Accueil > Déjà culte > Scouts et Guides en Belgique, Accueil > Déjà culte > Scouts Unitaires de France, Accueil > Déjà culte > Souvenirs du Monde, Accueil > Déjà culte > Souvenirs LaToileScoute, Accueil > Culture > Textes scouts de référence, Accueil > Culture > Le scoutisme, en musique, Accueil > Camper & Randonner > Partir en camp scout, Accueil > Camper & Randonner > Partir à l’aventure, Accueil > Camper & Randonner > Installations scoutes, Accueil > Camper & Randonner > Tests de matériels, Accueil > Camper & Randonner > Orientation, Accueil > Animer > Secrets de chefs scouts, Accueil > Créer > Objets Scouts Non Identifiés, Accueil > Services > Formations LaToileScoute, Accueil > Services > Utiles pour communiquer, Accueil > Services > Utiles pour s’informer, Accueil > Services > Utiles pour s’organiser, Accueil > L’association > Sous LaToileScoute, Accueil > L’association > Sur LaToileScoute, Accueil > L’association > L’histoire de LaToileScoute, Accueil > L’association > Soutenir ou contacter LaToileScoute, Par NASA, ESA Credit : A. Fujii [Public domain], via Wikimedia Commons, Par Till Credner (Travail personnel : AlltheSky.com) [CC BY-SA 3.0 (, http://creativecommons.org/licenses/by-sa/3.0, Droit de reproduction libre sous certaines conditions, © LaToileScoute, Association loi 1901, 2001 - 2020, Constellations de l’Aigle, du Cygne et de la Lyre, NASA, ESA Credit : A. Fujii [Public domain], via Wikimedia Commons, Till Credner (Travail personnel : AlltheSky.com) [CC BY-SA 3.0 (. It has the traditional name Sheliak, derived from šiliyāq, which is the Arabic name for the constellation. The sunlike star has a planet with over 6 Jupiter masses discovered in 2001, the second found in a triple system after that of 16 Cygni. The central star itself is a white dwarf with a temperature of 120,000 kelvins. Each such radial pulsation causes the star’s radius to vary from 5.1 to 5.6 times the solar radius. Lesley Brown: The New Shorter Oxford English Dictionary. Lyra represents the lyre of Orpheus, the musician and poet in Greek mythology who was killed by the Bacchantes. La constellation Lyra contient plusieurs étoiles brillantes qui dessinent sa forme. [79] Also discovered by the transit method is WASP-3b, with 1.75 times the mass of Jupiter. It is one of 48 listed by the 2nd century astronomer Ptolemy, and is one of the 88 constellations recognized by the International Astronomical Union. Image: Hubble Heritage Team. Lyre - Lyra - Lyr. Beginning at the north, Lyra is bordered by Draco, Hercules, Vulpecula, and Cygnus. en été, elle est presque au zénith Gamma Lyrae is the second brightest star in the constellation. The constellation contains six formally named stars. δ Lyrae est une étoile triple. Zeus sent an eagle to get the lyre and placed both of them in the sky. Function: require_once, Message: Undefined variable: user_membership, File: /home/ah0ejbmyowku/public_html/application/views/user/popup_modal.php La Lyre était lune des 48 constellations identifiées par Ptolémée. Elle permit à Orphée de vaincre les puissances des ténèbres avant de gagner le ciel à sa mort. La Lyre est visible de mai à novembre. Ce sont en fait des systèmes d'étoiles doubles dont les composantes s'éclipsent mutuellement à intervalles réguliers et qui sont suffisamment proches l'une de l'autre pour être sérieusement déformées par les forces de marée. la lyre est une constellation assez connue des astronomes amateurs. Line: 24 [82] Almost as sparse is Kepler-8b, only slightly more massive and of a similar radius. [64], Another planetary nebula in Lyra is Abell 46. The star names approved by the International Astronomical Union (IAU) are Aladfar, Sheliak, Sulafat, Vega, Xihe, and Chasoň. Their orbital period is about half that of the Epsilon-1 stars. The star has a mean apparent magnitude of 7.195 and is approximately 860 light years distant from the Sun. Mystery Star Cluster Has 3 Different Birthdays", "Most Earthlike planets yet seen bring Kepler closer to its holy grail", Warburg Institute Iconographic Database (over 180 medieval and early modern images of Lyra), https://en.wikipedia.org/w/index.php?title=Lyra&oldid=983079460, Wikipedia articles incorporating a citation from the 1911 Encyclopaedia Britannica with Wikisource reference, Creative Commons Attribution-ShareAlike License, This page was last edited on 12 October 2020, at 03:29. ε Lyrae est très connue pour être en fait une double double : ε1 et ε2 sont toutes deux des étoiles doubles dont les membres sont dans les deux cas séparés par 140 ua. 1: A−M. Vega, Lyra's brightest star, is one of the brightest stars in the night sky, and forms a corner of the famed Summer Triangle asterism. The components have apparent magnitudes of 5.569 and 9.8. [36] It can be found less than a degree away from the naked-eye star 16 Lyrae, a 5th-magnitude A-type subgiant[37] located around 37 parsecs distant. It and a likely companion are surrounded by a circumstellar disk of material. The brightest star in the constellation is Vega, Alpha Lyrae, which is also the fifth brightest star in the sky, with an apparent magnitude of 0.03. Delta Lyrae consists of a star and a star system sharing the same Bayer designation. Vol. Joining Jason and the Argonauts, his music was able to quell the voices of the dangerous Sirens, who sang tempting songs to the Argonauts. NGC 6745 is really a triplet of galaxies that have been colliding and merging for hundreds of millions of years. Lyra ou La Lyre est l'une des 88 constellations qui divisent le ciel selon les travaux des astronomes modernes. When galaxies collide, the stars that normally comprise the major portion of the luminous mass of each of the two galaxies will almost never collide with each other, but will pass rather freely between each other with little damage. La constellation de la Lyre est composée de dizaines d'étoiles dont la plus brillante est Véga. La lyre représenterait pour sa part l'instrument de musique d'Orphée. There are three meteor showers associated with the constellation: the Lyrids, which peak around April 21-22 every year, the June Lyrids and the Alpha Lyrids. [54] Originally classified as a VY Sculptoris star due to spending most time at maximum brightness, since around 1979 the system has been dominantly at minimum brightness, with periodic outbursts.
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