Eta Carinae is the most prominent variable star in Carina, with a mass of approximately 100 solar masses and 4 million times as bright as the Sun. [3] It was first discovered to be unusual in 1677, when its magnitude suddenly rose to 4, attracting the attention of Edmond Halley. [6] Eta Carinae is inside NGC 3372, commonly called the Carina Nebula. [3] It had a long outburst in 1827, when it brightened to magnitude 1, only fading to magnitude 1.5 in 1828. Its most prominent outburst made Eta Carinae the equal of Sirius; it brightened to magnitude −1.5 in 1843. In the decades following 1843 it appeared relatively placid, having a magnitude between 6.5 and 7.9. [6] However, in 1998, it brightened again, though only to magnitude 5.0, a far less drastic outburst. Eta Carinae is a binary star, with a companion that has a period of 5.5 years; the two stars are surrounded by the Homunculus Nebula, which is composed of gas that was ejected in 1843. [3] Caringbah South is a small district made up mostly of small businesses specialising in professional services. The blistering, ultraviolet radiation from the young stars is sculpting the nebula’s wall by slowly eroding it away. Dramatic pillars tower above the glowing wall of gas, resisting this radiation. The “steam” that appears to rise from the celestial “mountains” is actually hot, ionized gas and hot dust streaming away from the nebula due to the relentless radiation.

sprovođenje zakonom predviđenih postupaka u cilju otkrivanja carinskih prekršaja, privrednih prestupa i krivičnih dela i podnošenje prijava tužilaštvu ili drugim nadležnim državnim organima;The nebula is one of the largest diffuse nebulae in our skies. Although it is four times as large as and even brighter than the famous Orion Nebula, the Carina Nebula is much less well known due to its location in the southern sky. It was discovered by Nicolas-Louis de Lacaille in 1752 from the Cape of Good Hope. a b c Car Repair Manual–Carina/Celica. Maidenhead, Berkshire, UK.: Autodata. pp.6–7, History and Identification. (1981). Carina is a standard kubernetes CSI plugin. Users can use standard kubernetes storage resources like storageclass/PVC/PV to request storage media. The key considerations of carina includes: HD 93129 is a triple star system of O-class stars in Carina. All three stars of HD 93129 are among the most luminous in the galaxy; [33] HD 93129 consists of two clearly resolved components, HD 93129 A and HD 93129 B, and HD 93129 A itself is made up of two much closer stars.

Samus, N. N.; Durlevich, O. V.; etal. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)" . Retrieved 2012-04-08. a b Williams, S. J.; etal. (November 2011). "Radial Velocities of Galactic O-type Stars. I. Short-term Constant Velocity Stars". The Astronomical Journal. 142 (5). 146. Bibcode: 2011AJ....142..146W. doi: 10.1088/0004-6256/142/5/146. Chu CP, Chen PP (April 2002). "Tracheobronchial injury secondary to blunt chest trauma: Diagnosis and management". Anaesth Intensive Care. 30 (2): 145–52. doi: 10.1177/0310057X0203000204. PMID 12002920.NASA explores the unknown in air and space, innovates for the benefit of humanity, and inspires the world through discovery. The third generation was first released in September 1981. This was the last Carina to use rear-wheel drive. The RWD Corona shared its chassis with this vehicle, with the Corona being updated the succeeding year. The 1800SE had power windows, and an 1800SE "Extra Edition" trim level was added. The Carina was famously used by private teams racing for Japan in the Dakar Rally in the two-wheel-drive class for both 1981 and 1982. The Carina managed to achieve four championships in the marathon class divisions.

Stars v. Dust in the Carina Nebula". European Southern Observatory. 29 August 2018 . Retrieved 30 August 2018. Wolf–Rayet star and Algol variable, V max = 6.33 m, V min = 6.52 m, P = 80.34d; one of the most luminous stars known a b c d Kuhn, Michael A.; etal. (January 2019). "Kinematics in Young Star Clusters and Associations with Gaia DR2". The Astrophysical Journal. 870 (1). 32. arXiv: 1807.02115. Bibcode: 2019ApJ...870...32K. doi: 10.3847/1538-4357/aaef8c. S2CID 119328315. See, e.g., Burnham, Jr, Robert (1978). Burnham's Celestial Handbook. New York: Dover. p.467. ISBN 978-0-486-23567-7. Carina contains Canopus, a white-hued supergiant that is the second-brightest star in the night sky at magnitude −0.72. Alpha Carinae, as Canopus is formally designated, is 313 light-years from Earth. Its traditional name comes from the mythological Canopus, who was a navigator for Menelaus, king of Sparta. [3]

This generation was released in May 1988. The exterior sheet metal received rounded contours, as was in line with the fashionable design of products at that time. The Surf (wagon) and Van versions also underwent a full model change to bring them in line with their siblings. 4S-Fi is an 1800cc engine type, 1600cc of the 4A-GE and the specification for higher-power higher-cam-4A-FHE car, 1500cc of the 5A-F type, 2000cc diesel-2C. The 3E engine was fitted to the 1500cc Van, which was also available with the 2000cc diesel 2C engine. [18] This article needs additional citations for verification. Please help improve this article by adding citations to reliable sources. Unsourced material may be challenged and removed. The Carina Nebula. Eta Carinae and the Keyhole Nebula are left of center, NGC 3324 is at upper right. Carina is known for its namesake nebula, NGC 3372, [8] discovered by French astronomer Nicolas-Louis de Lacaille in 1751, which contains several nebulae. The Carina Nebula overall is an extended emission nebula approximately 8,000 light-years away and 300 light-years wide that includes vast star-forming regions. [9] It has an overall magnitude of 8.0 [6] and an apparent diameter of over 2 degrees. [3] Its central region is called the Keyhole, or the Keyhole Nebula. This was described in 1847 by John Herschel, and likened to a keyhole by Emma Converse in 1873. [10] The Keyhole is about seven light-years wide and is composed mostly of ionized hydrogen, with two major star-forming regions. The Homunculus Nebula is a planetary nebula visible to the naked eye that is being ejected by the erratic luminous blue variable star Eta Carinae, the most massive visible star known. Eta Carinae is so massive that it has reached the theoretical upper limit for the mass of a star and is therefore unstable. It is known for its outbursts; in 1840 it briefly became one of the brightest stars in the sky due to a particularly massive outburst, which largely created the Homunculus Nebula. Because of this instability and history of outbursts, Eta Carinae is considered a prime supernova candidate for the next several hundred thousand years because it has reached the end of its estimated million-year life span. [9] Garner, Rob (8 July 2022). "NASA Shares List of Cosmic Targets for Webb Telescope's 1st Images". NASA . Retrieved 8 July 2022.