Universe Guide


HD 196885, HIP101966

HD 196885 is a blue to white subgiant star that can be located in the constellation of Delphinus. HD 196885 is the brightest star in Delphinus based on the Hipparcos 2007 apparent magnitude. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it. The star has an estimated age of 6.80 Billion of Years but could be as young as 5.30 to 7.50 according to Hipparcos.

HIP101966 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD196885. HD 196885 has at least 1 Extrasolar Planets believed to be in orbit around the star.

Location of HD 196885

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 HD 196885, the location is 20h 39m 51.85 and +11d14`58.0 .

Proper Motion of HD 196885

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 83.87 ± 0.27 miliarcseconds/year towards the north and 47.34 ± 0.48 miliarcseconds/year east if we saw them in the horizon.

Physical Properties (Colour, Temperature, Age, Radius) of HD 196885

HD 196885 has a spectral type of F8IV:. This means the star is a blue to white subgiant star. The star is 7382.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24077.3780540800000000s. The star has a B-V Colour Index of 0.55 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 6,082 Kelvin.

HD 196885 Radius has been calculated as being 1.46 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,016,851.87.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 1.49. 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 0.17 with an error value of 0.02 Fe/H with the Sun has a value of 1 to put it into context.

The stars age according to Hipparcos data files put the star at an age of about 6.80 Billion years old but could be between 5.30 and 7.50 Billion years old. In comparison, the Sun's age is about 4.6 Billion Years Old.

HD 196885 Apparent and Absolute Magnitudes

HD 196885 has an apparent magnitude of 6.39 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 3.80 If you used the 2007 Parallax value, you would get an absolute magnitude of 3.76. 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 HD 196885

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 30.31 which gave the calculated distance to HD 196885 as 107.61 light years away from Earth or 32.99 parsecs. It would take a spaceship travelling at the speed of light, 107.61 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 29.83 which put HD 196885 at a distance of 109.34 light years or 33.52 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 7,382.00 Parsecs or 24,077.38 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

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.

HD 196885 Facts

Alternative Names

Traditional/Proper NameHD 196885
Hipparcos Library I.D.101966
Bonner DurchmusterungBD+10 4351
Henry Draper Designation196885

Visual Facts

Star Typesubgiant star
Age6.80 Billion Years Old
Age Range5.30 - 7.50 Billion Years Old
Absolute Magnitude3.80 / 3.76
Visual / Apparent Magnitude6.39
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)20h 39m 51.85
Declination (Dec.)+11d14`58.0
Galactic Latitude-17.99 degrees
Galactic Longitude56.31 degrees
1997 Distance from Earth30.31 Parallax (milliarcseconds)
 107.61 Light Years
 32.99 Parsecs
2007 Revised Distance from Earth29.83 Parallax (milliarcseconds)
 109.34 Light Years
 33.52 Parsecs
Galacto-Centric Distance24,077.38 Light Years / 7,382.00 Parsecs
Proper Motion Dec.83.87 ± 0.27 milliarcseconds/year
Proper Motion RA.47.34 ± 0.48 milliarcseconds/year
B-V Index0.55
Radial Velocity-30.13 ± 0.09 km/s
Iron Abundance0.17 ± 0.02 Fe/H
Spectral TypeF8IV:
Colour(F) blue to white

Companions (Multi-Star and Exoplanets) Facts

Exoplanet Count1

Estimated Facts

Calculated Effective Temperature6,082 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
196885+10 4351.0A6.4000073.0000091.00000F8Yellow/White

List of Extrasolar Planets orbiting HD 196885

NameStatusMass (Jupiters)Orbital Period (Days)EccentricityDiscoveredSemi-Major AxisPeriastron
Hd 196885 A BConfirmed2.981326.0000.4820072.693.000

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