Universe Guide

Tau1 Aquarii (69 Aquarii) Star Facts

Tau1 Aquarii Facts

  • Tau1 Aquarii is a main sequence star that can be located in the constellation of Aquarius. The description is based on the spectral class.
  • Tau1 Aquarii is not part of the constellation outline but is within the borders of the constellation.
  • Based on the spectral type (B9V) of the star, the star's colour is blue .
  • The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
  • Using the most recent figures given by the 2007 Hipparcos data, the star is 317.59 light years away from us. Distance

Tau1 Aquarii's Alternative Names

Tau1 Aquarii (Tau01 Aqr) is the Bayer Classification for the star. The Bayer Classification was created by Johann Bayer in 1603. The brightest star in the constellation is normally given the Alpha designation, there are exceptions such as Pollux which is Beta Geminorum.

The Id of the star in the Yale Bright Star Catalogue is HR8673. HIP112542 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD215766.

Flamsteed designations are named after the creator, Sir John Flamsteed. Sir John named the stars in the constellation with a number and its latin name, this star's Flamsteed designation is 69 Aquarii. The Flamsteed name can be shortened to 69 Aqr.

The Gould star designation is one that was designed by American astronomer, Benjamin Apthorp Gould. Gould stars are predominantly in the Southern and Equatorial constellations but do appear in northern constellations such as Bootes and Orion. The star has the designation 180 G. Aquarii. There are no stars with a Gould designation in Ursa Major for example.

BD number is the number that the star was filed under in the Durchmusterung or Bonner Durchmusterung, a star catalogue that was put together by the Bonn Observatory between 1859 to 1903. The star's BD Number is BD-14 6346.

More details on objects' alternative names can be found at Star Names .

Location of Tau1 Aquarii

The location of the main sequence star in the night sky 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 object is compared to the celestial equator and is expressed in degrees. For Tau1 Aquarii, the location is 22h 47m 42.75 and -14° 03` 23.1 .

Radial Velocity and Proper Motion of Tau1 Aquarii

Proper Motion

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 -9.23 ± 0.27 milliarcseconds/year towards the north and 30.61 ± 0.46 milliarcseconds/year east if we saw them in the horizon.

Radial Velocity

The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is 15.00000 km/s with an error of about 3.70 km/s . When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever.

Physical Properties of Tau1 Aquarii

Tau1 Aquarii Colour and Temperature

Based on the star's spectral type of B9V , Tau1 Aquarii's colour and type is blue main sequence star. The star has a B-V Colour Index of -0.01 which means the star's temperature is about 9,679 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu.

Tau1 Aquarii Luminosity

Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. The figure of 52.62 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.

Tau1 Aquarii Radius

Tau1 Aquarii estimated radius has been calculated as being 1.94 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,348,079.06.km. If you need the diameter of the star, you just need to multiple the radius by 2. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 2.3617567274613280281045990088. The figure is derived at by using the formula from SDSS rather than peer reviewed papers. It has been known to produce widely incorrect figures.

Tau1 Aquarii Apparent and Absolute Magnitudes

Tau1 Aquarii has an apparent magnitude of 5.68 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 1.17 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.74. 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 Tau1 Aquarii

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 12.55000 which gave the calculated distance to Tau1 Aquarii as 259.89 light years away from Earth or 79.68 parsecs. If you want that in miles, it is about 1,527,795,948,236,688.40, based on 1 Ly = 5,878,625,373,183.61 miles.

In 2007, Hipparcos data was revised with a new parallax of 10.27000 which put Tau1 Aquarii at a distance of 317.59 light years or 97.37 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.

Using the 2007 distance, the star is roughly 20,083,864.24 Astronomical Units from the Earth/Sun give or take a few. An Astronomical Unit is the distance between Earth and the Sun. The number of A.U. is the number of times that the star is from the Earth compared to the Sun. The star's Galacto-Centric Distance is 7,369.00 Parsecs or 24,034.98 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Travel Time to Tau1 Aquarii

The time it will take to travel to this star is dependent on how fast you are going. U.G. has done some calculations as to how long it will take going at differing speeds. A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).

The New Horizons space probe is the fastest probe that we've sent into space at the time of writing. Its primary mission was to visit Pluto which at the time of launch (2006), Pluto was still a planet.

DescriptionSpeed (m.p.h.)Time (years)
Airbus A380736289,376,542.40
Speed of Sound (Mach 1)767.269277,583,396.70
Concorde (Mach 2)1,534.54138,791,517.46
New Horizons Probe33,0006,453,973.79
Speed of Light670,616,629.00317.59

Meteor Showers Radiating from near Tau1 Aquarii

The Tau Aquariids Meteor Shower radiants from a point near this star. The meteor shower runs typically between 27 Jun- 6 Jul with a peak date of 28-Jun. The speed of a meteor in the shower is 64 Km/s. The amount of meteors predicted to be seen per hour (Zenith Hourly Rate) is 64.

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.

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Additional Tau1 Aquarii Facts and Figures

Visual Facts

Primary / Proper / Traditional NameTau1 Aquarii
Alternative NamesTau01 Aqr, HD 215766, HIP 112542, HR 8673, 180 G. Aquarii, 69 Aquarii, 69 Aqr, BD-14 6346
Spectral TypeB9V
Constellation's Main StarNo
Multiple Star SystemYes
Star Type Main Sequence Dwarf Star
GalaxyMilky Way
Absolute Magnitude 1.17 / 0.74
Visual / Apparent Magnitude5.68
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)22h 47m 42.75
Declination (Dec.)-14° 03` 23.1
Galactic Latitude-58.35404399 degrees
Galactic Longitude51.06223699 degrees
1997 Distance from Earth12.55000 Parallax (milliarcseconds)
 259.89 Light Years
 79.68 Parsecs
2007 Distance from Earth10.27000 Parallax (milliarcseconds)
 317.59 Light Years
 97.37 Parsecs
 20,083,864.24 Astronomical Units
Galacto-Centric Distance24,034.98 Light Years / 7,369.00 Parsecs
Proper Motion Dec.-9.23000 ± 0.27000 milliarcseconds/year
Proper Motion RA.30.61000 ± 0.46000 milliarcseconds/year
B-V Index-0.01
Radial Velocity15.00000 ± 3.70 km/s
Semi-Major Axis8394.0000000
Stellar Luminosity (Lsun)52.6200000
Associated / Clustered StarsTau2 Aquarii

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Estimated Calculated Facts

Radius (x the Sun)2.36
Effective Temperature9,679 Kelvin

Sources and Links

SIMBAD SourceLink

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
215766-14 6346.0A5.8000029.00000-5.00000B9Blue/White

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