The wordgames anagrams, crossword, Lettris and Boggle are provided by Memodata. Longitude: 0° 00’ 00” E Likewise, Sirius is Alpha Canis Majoris, the "A" star of Canis Major, and Pishpai is Mu Geminorum, the "M" star of Gemini. The brightest star in the constellation is normally given the Alpha designation, there are exceptions such as Pollux which is Beta Geminorum.
By using our services, you agree to our use of cookies. Ces noms sont pour la plupart dérivés de phrases en arabe ou en latin décrivant la position de l étoile à l intérieur de leur constellation, ce qui explique également qu il y …   Wikipédia en Français, Mu Arae — Observation data Epoch J2000.0      Equinox J2000.0 …   Wikipedia, Capella (star) — For other uses, see Capella (disambiguation). A windows (pop-into) of information (full-content of Sensagent) triggered by double-clicking any word on your webpage. An Astronomical Unit is the distance between Earth and the Sun. Iota Canis Majoris has an apparent magnitude of 4.36 which is how bright we see the star from Earth. It is emitting 3,603[9] times the luminosity of the Sun and is a suspected Beta Cephei variable. Iota Ursae Majoris — A/B/C Données d observation (Époque J2000) Ascension droite 08h 59m 12.4s Déclinaison +48° 02′ 30″ Constellation Grande Ourse Magnitude apparente 3,12/10,1/10 …   Wikipédia en Français, Iota Ursae Majoris — Datenbanklinks zu Iota Ursae Majoris Stern ι Ursae Majoris …   Deutsch Wikipedia, Iota Coronae Borealis — Constelación Corona Boreal Ascensión recta α 16h 01min 26,56s Declinación δ +29º 51’ 03,8’’ Distancia …   Wikipedia Español, Nu² Canis Majoris — For other star systems with this Bayer designation, see Nu Canis Majoris.

Ye una estrella distante asitiada a 2500 ± 250 años lluz del Sistema Solar.. Iota Canis Majoris ye una estrella blancu-azulada de tipu espectral B3Ib-II con carauterístiques entemedies ente superxigante «menor» y una xigante lluminosa.

Telting, J. H. et al. [4] This energy is being radiated from its outer envelope at an effective temperature of about 18,700 K,[9] giving it the blue-white hue of a B-type star. The SensagentBox are offered by sensAgent. If you find this website useful please consider a small donation that will help covering hosting costs. See if you can get into the grid Hall of Fame ! Iota Canis Majoris estimated radius has been calculated as being 26.72 times bigger than the Sun. Give contextual explanation and translation from your sites !

English thesaurus is mainly derived from The Integral Dictionary (TID).

Iota Canis Majoris (ι Canis Majoris, ι CMa) is a variable supergiant star in the constellation Canis Major.. Iota Canis Majoris is a blue-white B-type supergiant with an apparent magnitude that varies between +4.36 and +4.40. By using our services, you agree to our use of cookies. Hohle, M. M.; Neuhäuser, R.; Schutz, B. F. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants". Each square carries a letter. Privacy policy The SensagentBox are offered by sensAgent.

(countable) A printed or computer-stored instance of that ninth letter. is the number of times that the star is from the Earth compared to the Sun. the Hertzsprung–Russell diagram. All rights reserved.

The red dot in the diagram below shows where ι Canis Majoris is situated in It is approximately 3100 light years from Earth. Di, Cookies help us deliver our services. The web service Alexandria is granted from Memodata for the Ebay search. Boggle gives you 3 minutes to find as many words (3 letters or more) as you can in a grid of 16 letters. ι Canis Majoris (iota Canis Majoris) ι Canis Majoris is a variable bright giant star in the constellation of Canis Major. Change the target language to find translations. van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction". OK. Talitha, Talitha Borealis, Alphikra Borealis, 9 Ursae Majoris, Gl 331, HR 3569, BD +48°1707, NightSky Friday: Rotanev, Derf, Navi, and other Backward Star Names. ○   Anagrams

To make squares disappear and save space for other squares you have to assemble English words (left, right, up, down) from the falling squares. ι Canis Majoris visual magnitude is 4.37. Using the most recent figures given by the 2007 Hipparcos data, the star is 2508.95 light years away from us.

Contact Us Canis Major is a constellation in the southern celestial hemisphere.In the second century, it was included in Ptolemy's 48 constellations, and is counted among the 88 modern constellations.Its name is Latin for "greater dog" in contrast to Canis Minor, the "lesser dog"; both figures are commonly represented as following the constellation of Orion the hunter through the sky.

Today's ι Canis Majoris (iota Canis Majoris) rise, transit and set times from Celestial coordinates for the J2000 equinox as well as galactic coordinates of ι Canis Majoris are provided in the following table: The simplified sky map below shows the position of ι Canis Majoris in the sky: Location: Greenwich, United Kingdom [change] The Bayer designation Zeta Canis Majoris was assigned by German astronomer Johann Bayer in 1603. Privacy policy

ν² Canis Majoris Observation data Epoch J2000.0      Equinox J2000.0 Constellation Canis Major Right ascension 06h36m41.0s …   Wikipedia, Dnoces — Iota Ursae Majoris Iota Ursae Majoris A/B/C Données d observation (Époque J2000) Ascension droite 08h 59m 12.4s Déclinaison +48° 02′ 30″ Constellation Grande Ourse Magnitude apparente …   Wikipédia en Français, Talitha Borealis — Iota Ursae Majoris Iota Ursae Majoris A/B/C Données d observation (Époque J2000) Ascension droite 08h 59m 12.4s Déclinaison +48° 02′ 30″ Constellation Grande Ourse Magnitude apparente …   Wikipédia en Français, Liste De Noms Traditionnels D'étoiles — Cette page donne une liste des noms traditionnels de certaines étoiles. Information regarding Metallicity and/or Mass is from the E.U. the credits section) taken in the red channel. noun verb masculine is from Simbad, the Hipparcos data library based at the University at Strasbourg, France. in the constellation of All messages will be reviewed before being displayed. Find out more.

3,075.47 light years from the Sun and it is Iota Canis Majoris (ι CMa / 20 Canis Majoris / HD 51309) ye una estrella na constelación del Can Mayor de magnitú aparente +4,39. For Iota Canis Majoris, the location is 06h 56m 08.23 and -17° 03` 15.3 . The brightest component, Iota Ursae Majoris A, is a white A-type subgiant with an apparent magnitude of +3.12. Apparent Magnitude is also known as Visual Magnitude. Evans, D. S. (June 20–24, 1966), "The Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; John Frederick. The companion binary is composed of the 9th magnitude Iota Ursae Majoris B and the 10th magnitude Iota Ursae Majoris C. These two stars orbit around each other with a period of 39.7 years, and are separated by roughly 0.7 arcseconds, or at least 10 AU. Your guide to the Solar System and the night sky. There's no register feature and no need to give an email address if you don't need to. Mach 1 is the speed of sound, Mach 2 is twice the speed of sound. Parallax measurements from the Hipparcos mission yield a distance estimate of around 362 ly (111 pc) from Earth. Iota Canis Majoris Facts. ι Canis Majoris is a blue-white B-type bright giant with a mean apparent magnitude of +4.36.

IOTA CMA (Iota Canis Majoris). Iota Canis Majoris, lying between Sirius and Gamma, is another star that has been classified as a Beta Cephei variable, varying from magnitude 4.36 to 4.40 over a period of 1.92 hours.

Davis Jr., G. A. Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. Cookies help us deliver our services. Boggle gives you 3 minutes to find as many words (3 letters or more) as you can in a grid of 16 letters. Each square carries a letter. The table below Add new content to your site from Sensagent by XML. By using our services, you agree to our use of cookies. Using the 2007 distance, the star is roughly 158,663,971.32 Astronomical Units from the Earth/Sun give or take a few. Choose the design that fits your site. The Sun's radius is 695,800km, therefore the star's radius is an estimated 18,590,487.96.km. Thank you! The star is moving 2.42 ± 0.15 milliarcseconds/year towards the north and -3.56 ± 0.20 milliarcseconds/year east if we saw them in the horizon. ○   Anagrams [13] The Bayer designation Zeta Canis Majoris was assigned by German astronomer Johann Bayer in 1603.
The apparent separation between the two binaries is rapidly decreasing as they follow their orbits. Letters must be adjacent and longer words score better.

for the next 100000 years is represented with the red arrow. If you want that in miles, it is about 18,088,589,059,539,699.81, based on 1 Ly = 5,878,625,373,183.61 miles. Change the target language to find translations. The brightest component, Iota Ursae Majoris A, is a white A-type subgiant with an apparent magnitude of +3.12. Iota Canis Majoris (Iot Cma) is the Bayer Classification for the star. The source of the information if it has a Hip I.D. Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun". from God’s true Christian religion in the earth; Him without his pure, undefiled religion in the earth. Cookies / About Us / Contact Us / Twitter / Facebook, Iot Cma, Iota CMa, HD 51309, HIP 33347, HR 2596, TYC 5967-2618-1, 20 Canis Majoris, 20 Cma, BD-16 1661. Iota Canis Majoris Iron Abundance is -0.04 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context. The English word games are:

In 2007, Hipparcos data was revised with a new parallax of 1.30000 which put Iota Canis Majoris at a distance of 2508.95 light years or 769.23 parsecs. Most English definitions are provided by WordNet . Canis Major. More details on objects' alternative names can be found at. See if you can get into the grid Hall of Fame ! The number of A.U. Company Information Iota Canis Majoris is a B3IB/II supergiant star based on the spectral type that was recorded in the Hipparcos star catalogue.