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70 Ophiuchi - HD165341 - HIP88601

70 Ophiuchi is a orange to red main sequence dwarf star that can be located in the constellation of Ophiuchus. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

HIP88601 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD165341. The Id of the star in the Gould Star Catalogue is 197. Stars in the southern hemisphere are more likely to have a Gould Id than the northern hemisphere. For example, there are no Gould classified stars in Ursa Major. The Gliese ID of the star is Gliese GL702A. The star was part of the original catalogue devised by German Astronomer Wilheim Gliese of stars located within 20 parsecs of Earth. Ref : Star Names.

70 Ophiuchi has alternative name(s), 70 Ophiuchi , V2391_Oph, 70 Oph. 70 Ophiuchi is a multiple star system with 2 stars orbiting in its solar system.

Location of 70 Ophiuchi

The location of the star in the galaxy is determined by the Right Ascension (R.A.) and Declination (Dec.), these are equivalent to the Longitude and Latitude on the Earth. The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. If the R.A. is positive then its eastwards. The Declination is how far north or south the star is compared to the celestial equator and is expressed in degrees. For 70 Ophiuchi, the location is 18h 05m 27.21 and +02d30`08.8 .

Proper Motion of 70 Ophiuchi

All stars like planets orbit round a central spot, in the case of planets, its the central star such as the Sun. In the case of a star, its the galactic centre. The constellations that we see today will be different than they were 50,000 years ago or 50,000 years from now. Proper Motion details the movements of these stars and are measured in milliarcseconds. The star is moving -962.82 ± 0.58 miliarcseconds/year towards the north and 124.16 ± 0.83 miliarcseconds/year east if we saw them in the horizon.

Physical Properties (Colour, Temperature, Radius) of 70 Ophiuchi

70 Ophiuchi has a spectral type of K0V SB. This means the star is a orange to red main sequence dwarf star. The star is 7396.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24123.0409222400000000s. The star has a B-V Colour Index of 0.86 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,141 Kelvin.

70 Ophiuchi Radius has been calculated as being 0.93 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 650,487.01.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 0.93. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures. The star's Iron Abundance is 0.03 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.

70 Ophiuchi Apparent and Absolute Magnitudes

70 Ophiuchi has an apparent magnitude of 4.03 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. If you used the 1997 Parallax value, you would get an absolute magnitude of 5.50 If you used the 2007 Parallax value, you would get an absolute magnitude of 5.50. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A faint star will have a high number.

Distance to 70 Ophiuchi

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 196.62 which gave the calculated distance to 70 Ophiuchi as 16.59 light years away from Earth or 5.09 parsecs. It would take a spaceship travelling at the speed of light, 16.59 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.

In 2007, Hipparcos data was revised with a new parallax of 196.72 which put 70 Ophiuchi at a distance of 16.58 light years or 5.08 parsecs. It should not be taken as though the star is moving closer or further away from us. It is purely that the distance was recalculated.

The star's Galacto-Centric Distance is 7,396.00 Parsecs or 24,123.04 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*. 70 Ophiuchi brightness ranges from a magnitude of 4.000 to a magnitude of 4.000 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 2.0 days (variability).

Source of Information

The source of the information if it has a Hip I.D. is from Simbad, the Hipparcos data library based at the University at Strasbourg, France. Hipparcos was a E.S.A. satellite operation launched in 1989 for four years. The items in red are values that I've calculated so they could well be wrong. Information regarding Metallicity and/or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.

70 Ophiuchi Facts

Alternative Names

Traditional/Proper Name70 Ophiuchi
Short NameV2391 Oph, 70 Oph
Alternative Name(s)70 Ophiuchi
Hipparcos Library I.D.88601
Bonner DurchmusterungBDD+02 3482
Gould I.D.197
Gliese ID702A
Henry Draper Designation165341

Visual Facts

Star Typemain sequence dwarf star
Absolute Magnitude5.50 / 5.50
Visual / Apparent Magnitude4.03
Naked Eye VisibleYes - Ref: Wiki
Right Ascension (R.A.)18h 05m 27.21
Declination (Dec.)+02d30`08.8
Galactic Latitude11.37 degrees
Galactic Longitude29.90 degrees
1997 Distance from Earth196.62 Parallax (milliarcseconds)
 16.59 Light Years
 5.09 Parsecs
2007 Revised Distance from Earth196.72 Parallax (milliarcseconds)
 16.58 Light Years
 5.08 Parsecs
Galacto-Centric Distance24,123.04 Light Years / 7,396.00 Parsecs
Proper Motion Dec.-962.82 ± 0.58 milliarcseconds/year
Proper Motion RA.124.16 ± 0.83 milliarcseconds/year
B-V Index0.86
Radial Velocity-6.87 ± 0.08 km/s
Iron Abundance0.03 ± 9.99 Fe/H
Spectral TypeK0V SB
Colour(K) Orange to Red
Stars in Solar System2

Variable Star Details

Mean Variability Period in Days2.000

Estimated Facts

Calculated Effective Temperature5,141 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

Multi-Star System

The star has been identified as being a multi-star system, one in which there is at least one star in close orbit to another star or two or more stars orbiting a central point. The stars may be of equal mass, unequal mass where one star is stronger than the other or be in groups orbiting a central point which doesn't necessarily have to be a star. More information can be found on my dedicated multiple star systems page. The source of the info is Simbad. The file is dated 2000 so any differences between this and any other source will be down to the actual source from where the information came from.


Proper Motion mas/yr
H.D. IdB.D. IdStar CodeMagnitudeR.A.Dec.SpectrumColourYear
165341+02 3482.0A4.30000261.00000-1100.00000K1Orange
B6.30000K6Orange1959
P13.0000012.00000-16.000001925
Q14.000001946
R13.000001946
S12.50000-10.00000-33.000001946
T13.100001946
U13.000001945
V11.800001.000000.000001946
VW12.600001906
VX13.500001906
Y14.100001924
BZ1900

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