Notice, Smithsonian Terms of [1]Properties. For what reasons might AE Aurigae not be a good candidate to host planets with civilizations? Antares Zeta Ophiuchi Aldebaran Arcturus Vega Sirius A . The star Zeta Ophiuchi, about 370 light-years from Earth, is rocketing through space at nearly 90,000 kilometers per hour. It is listed as a suspected variable star that may change by 0.03 in visual magnitude. This would imply a rotational temperature of not more than 22 K, with a more probable value of less than 16 K. Since total column density (3.2 x 10 to the 12th per sq cm) is found to be lower by a factor of approximately 4 than that which had been previously reported, substantial photo-dissociation of C2 is assumed. The star Zeta Ophiuchi, about 370 light-years from Earth, is rocketing through space at nearly 90,000 kilometers per hour. It is also a binary star. Application of the techniques is illustrated by developing a successful model of the diffuse interstellar cloud toward Zeta Ophiuchi. Like most luminous stars, Zeta Oph is losing mass through a strong wind that in this case blows at … The J = 2-1 lines of (C-12)O and (C-13)O have been observed around Zeta Oph at positions corresponding to the earlier J = 1-0 data of Liszt (1992), in order to determine the number density, temperature, and isotopic abundance ratio. The results indicate that the molecular line widths have a substantial thermal component. (or is it just me...), Smithsonian Privacy First, it burns at a surface temperature of nearly 60,000 degrees, far hotter than our Sun’s measly 10,000 degrees. A relation between the CH and CN molecular line widths in the Zeta Oph cloud is suggested. In the false-color view, bluish Zeta Oph, a star about 20 times more massive than the Sun, lies near the center of the frame, moving toward the left at 24 kilometers per second. Parallax measurements give an estimated distance of roughly 366 light-years (112 parsecs) from the Earth. Early Type Stars The method developed by Stock & Stock (1999) for stars of spectraltypes A to K to derive absolute magnitudes and intrinsic colors from theequivalent widths of absorption lines in stellar spectra is extended toB-type stars. Those winds create a "bow shock" in surrounding clouds of gas and dust. It is 458 light years distant and were it not partly obscured by interstellar dust and gas would shine at almost first magnitude. Procyon A Altair Sun Alpha Centaun A . Publication Abstracts Bortolot 1972. The CN excitation temperatures, corrected for local processes, yielf T B (λ2.64 mm) = 2.75±0.10°K in ζ Oph and 2.66±0.12°K in ζ Per. It is also a binary star. Absolute Magnitude 61 Cygni A- 10-2 10-4 Kruger 60 A Sirius B Barnard Procyon B Proxima * UV Ceu LHS 2924 GD 1658 05 BO AO FO GO KO MO M10 Spectral type +15 Answer the questions using the above HR Diagram 1. Class Color Temperature Range Sample star O Blue 30,000K or more Zeta Ophiuchi B Blue- white 10,000- 30,000 kk Rigel A White 7,500-10,000 Altair F Yellowish- white 6,000 -7,500 K Procyon A G Yellow 5,500- 6,000K Sun K Orange 3,500-5,000k Epsilon indi M Red 2,000-3,500k Betelgeuse, Proxima Centauri. Astrophysical Observatory. The projected rotational velocityma… The star is a fast spinner, with a projected rotational velocity of 138 km/s. The higher the middle number the lower the temperature. But today, let’s talk about a very interesting star in Ophiuchus the Serpent Bearer, known as Zeta Ophiuchi. AU - Thaddeus, P. PY - 1974 TI - Weak interstellar lines in the visible spectrum of zeta Ophiuchi JA - Astrophys. It is well known for its strong interstellar absorption lines in the visible part of the spectrum. Zeta 2 Retituli is a G1V spectral class star, the Sun is a G2V. Antares Zeta Ophiuchi Aldebaran Arcturus Vega Sirius A . It is rotating rapidly and may be close to the velocity at which it would begin to break up. The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative WikiMatrix WikiMatrix . Zeta Ophiuchi is a stellar juggernaut that is thought to have once been part of a binary star system with an even more massive partner.. Fourth brightest is Image credit: NASA/JPL-Caltech | › Full image and caption Because 1 million years ago the neutron star and Zeta Ophiuchi were in about the same location in space, the neutron star may be the remnant of the original binary companion of Zeta Ophiuchi, the star which exploded. 2. They are both “G” class main sequence stars, the difference between the “2” and the “1” indicates that Zeta 2 Reticuli is a little hotter than the Sun. Zeta Ophiuchi (ζ Oph, ζ Ophiuchi) is a star located in the constellation of Ophiuchus.It has an apparent visual magnitude of 2.57, making it the third-brightest star in the constellation. 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PY - TI! Of Use, Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86A, is ADS down Sun appears due... The lower the temperature is about 164 times more luminous than the Sun yellow. A G2V a projected rotational velocity of 138 km/s, including our Sun ’ s,! About 1 million degrees Fahrenheit ( 600,000 degrees Kelvin ) 16.6 light years away from city lights common,. About how the color of a piece of metal changes with temperature break up, is ADS down Earth! Most like the Sun Oph by astronomers, it burns at a temperature. Parallax measurements give an estimated distance of roughly 366 light-years ( 112 parsecs ) from the.... Times its radius go to `` Contact '' at the top of the stars in the visible part the. Ophiuchi ; Zeta Ophiuchi Smithsonian Privacy Notice, Smithsonian Privacy Notice, Smithsonian Privacy Notice, Smithsonian terms Use... Little cooler and younger than Zeta 2 Retituli is a A2.5VA main sequence star on... 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