This data is the best data we have at this time about Zeta 1 & 2 Reticuli.
It is long, but bear along, and the links are given to where the data was obtained from.
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Zeta(2) Reticuli: 39.3952 light-years, class G1 V
Zeta(1) Reticuli: 39.5288 light-years, class G2 V
Zeta 2:
Spectral class: G1
Luminosity Class: V
Apparent visual magnitude: +5.24
Absolute visual magnitude: +4.83
Visual luminosity: 1.020 x Sol
Color indices: B-V= +0.60
Mass: 1 x Sol
Diameter: 0.987 x Sol
Source for diameter: Apparent Diameters and Absolute Radii of Stars (Fracassini+ 1988)
Comfort Zone (visual): 1.010 A.U.s
Orbital period in CZ: 1.01469 years
Tidal index in CZ: 0.971251
Angular size of star in sky in CZ: 0.520878 degrees
Proper names: Zeta(2) Reticuli, Zeta Reticuli
Catalog numbers:
Gliese (Gl) 138, Henry Draper (HD) 20807, Cape Photographic Durchmusterung (CPD) -62°265 , Luyten Half-Second (LHS) 172 , Hipparcos Input Catalog
(HIC) 15371, Smithsonian Astrophysical Observatory (SAO) 248774, Hoffleit Bright Star (HR) 1010, Luyten Two-Tenth (LTT) 1576
Age: 8700 million years
Source for age: B. Edvardsson et al., "Chemical Evolution of the Galactic Disc", A&AP 275
Heavy element abundance: 73% of Sol
Standard error in heavy element abundance: 21%
Source for heavy element abundance: Strobel [Fe/H] Determinations
Arity: singular
Points of interest:
This star and Zeta(1) Reticuli may actually form a binary system. If so, the two stars are at least 5500 A.U. apart in space, which would give them a
very very long orbital period.
B. Edvardsson et al. arrived at a metallicity of 55% of Sol for this star, based on their measured iron-to-hydrogen ratio of 59% of the Solar value.
Right Ascension and Declination: 3h18m12.81s, -62°30'23" (epoch 2000.0)
Distance from Sol: 39.40 light-years (12.08 parsecs)
Standard error in distance: 0.6361%
Source for distance: Hipparcos
Celestial (X,Y,Z) coordinates in ly: 11.80, 13.84, -34.95
Galactic (X,Y,Z) coordinates in ly: 4.025, -26.44, -28.93
Proper motion: 1.483 arcsec/yr (63.7° from north)
Radial Velocity: 11.5 km/sec
Source for proper motion and radial velocity: Gliese
Galactic (U,V,W) velocity components in km/s: -70.05, -46.35, 16.94
www.stellar-database.com...
Zeta 1:
Spectral class: G2
Luminosity Class: V
Apparent visual magnitude: +5.53
Absolute visual magnitude: +5.11
Visual luminosity: 0.786 x Sol
Color indices: B-V= +0.64
Mass: 0.9 x Sol
Diameter: 0.912 x Sol
Source for diameter: Apparent Diameters and Absolute Radii of Stars (Fracassini+ 1988)
Comfort Zone (visual): 0.887 A.U.s
Orbital period in CZ: 321.369 days
Tidal index in CZ: 1.29173
Angular size of star in sky in CZ: 0.548307 degrees
Proper names: Zeta(1) Reticuli, Zeta Reticuli
Catalog numbers:
Gliese (Gl) 136, Henry Draper (HD) 20766, Cape Photographic Durchmusterung (CPD) -63°217 , Luyten Half-Second (LHS) 171 , Hipparcos Input Catalog
(HIC) 15330, Smithsonian Astrophysical Observatory (SAO) 248770, Hoffleit Bright Star (HR) 1006
Heavy element abundance: 71% of Sol
Standard error in heavy element abundance: 21%
Source for heavy element abundance: Strobel [Fe/H] Determinations
Arity: singular
Points of interest:
This star and Zeta(2) Reticuli may actually form a binary system. If so, the two stars are at least 5500 A.U. apart in space, which would give them a
very very long orbital period.
Right Ascension and Declination: 3h17m46.12s, -62°34'30.1" (epoch 2000.0)
Distance from Sol: 39.53 light-years (12.12 parsecs)
Standard error in distance: 0.6502%
Source for distance: Hipparcos
Celestial (X,Y,Z) coordinates in ly: 11.84, 13.83, -35.09
Galactic (X,Y,Z) coordinates in ly: 4.097, -26.52, -29.02
Proper motion: 1.495 arcsec/yr (63.2° from north)
Radial Velocity: 12.2 km/sec
Source for proper motion and radial velocity: Gliese
Galactic (U,V,W) velocity components in km/s: -71.24, -46.81, 16.08
www.stellar-database.com...
What do these fields mean?
www.stellar-database.com...
Comfort Zone: This is the distance, in Astronomical Units, at which we're pretty sure a planet may orbit this star and support life on its
surface. (One Astronomical Unit is the mean distance from the Earth to the sun.) Much closer and the life forms would fry, or the air and water would
evaporate; much further and life forms would freeze. Note that, since humankind has only ever stumbled across one planet where we know for sure that
life exists, it's hard to generalize about the range of conditions under which life as we know it could arise; thus, the comfort "zone" is listed
as a single distance, being the distance a planet would have to be from the star to receive precisely as much light as the Earth does from the sun.
Note also that even if an Earth-like planet were present at the comfort zone distance, other factors could make such a planet uninhabitable (like if
the star occasionally emits large, lethal flares).
The comfort zone distance in A.U.s is computed by simply taking the square root of the star's luminosity in solar units, since the light received by
a planet falls off with the square of its distance from the star. In the Internet Stellar Database, I've cheated a little bit by using the visual
luminosity (the luminosity passing through a filter that approximates our own eyes' bias) as the basis for the comfort zone. This is reasonable for
yellowish stars like our sun, but doesn't work as well for very cool or very hot stars. Cool red stars tend to emit more of their energy in the
infrared portion of the spectrum, while hot blue stars tend to emit more energy at frequencies higher than the visual "peak" frequency. I should
really be using the bolometric luminosity (the energy emitted at all frequencies), but bolometric data are pretty hard to find for most stars.
Orbital period in CZ: If a planet, whose mass was small compared with the star, were in a circular orbit about this star in its comfort zone,
this entry shows how long the "year" on that planet would be. (This figure is related both to the distrance the planet is from the star and the mass
of the star itself. More massive stars demand faster orbits, but greater distances both take longer to traverse and require that the orbiting object
be moving more slowly.) The exact relationship for a planet orbiting at any distance is P2 = A3/M, where M is the mass of the star in solar masses, P
is the orbital period in Earth years, and A is the semimajor axis (radius) of the orbit in Astronomical Units. Conveniently, for the Earth's orbit
around the sun, all three of these values — P, A, and M — are equal to 1.
Tidal Index in CZ: If a planet were in a circular orbit about this star in its comfort zone, this entry shows how strong the star's tidal
forces would be on said planet, relative to the strength of the Sun's tidal forces on Earth. A very high Tidal Index means that any such planet would
quickly become locked in synchronous rotation around the star, so that the same side of the planet faces the star at all times (in the same way that
the moon is locked in synchrorous rotation around the Earth).
Angular size in sky in CZ: If a planet were in a circular orbit about this star in its comfort zone, this entry shows how big the star would
appear to an observer on the surface of said planet. The Earth's sun subtends an angle of about 0.5 degrees.
Detected companions: If any actual planets or brown dwarfs have been detected around this star, directly or indirectly, the number so
discovered will be mentioned here. The "Points of Interest" field (above) will likely have a more in-depth description as to what is known about
these unseen objects.
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Now:
Zeta 2:
Mass: 1 x Sol
Diameter: 0.987 x Sol
Source for diameter: Apparent Diameters and Absolute Radii of Stars (Fracassini+ 1988)
Comfort Zone (visual): 1.010 A.U.s
Orbital period in CZ: 1.01469 years
Tidal index in CZ: 0.971251
Angular size of star in sky in CZ: 0.520878 degrees
Comfort Zone would be compared to Earth around our Sun (Sol) 1.010 A.U. s units or 1 A.U. is 93,000,000 miles between the Earth and Sun, so a planet
they think to be in a CZ around Zeta 2 would be slightly further away than Earth is from our Sun -- or 1.010 times 93,000,000 miles.
Zeta 1:
Mass: 0.9 x Sol
Diameter: 0.912 x Sol
Source for diameter: Apparent Diameters and Absolute Radii of Stars (Fracassini+ 1988)
Comfort Zone (visual): 0.887 A.U.s
Orbital period in CZ: 321.369 days
Tidal index in CZ: 1.29173
Angular size of star in sky in CZ: 0.548307 degrees
For Zeta 1, an Earth like planet should be only the CZ of 0.887 AU. or closer to that Sun than our Earth is to our Sun away, so 0.887 times 93,000,000
miles away for a habitable planet.
This is the best known data about that star system!
The stars do orbit around one another in a very long orbital period. However that is hard to determine as it may take many years of our time to really
figure that out.
Orbital period is for an Earth-like planet and the length of the year --- or 321.369 days and 1.01469 years compared to our 365.2522 days around our
Sun for the Earth!
A planet has to be in a Critical Zone Distance away from a Sun, or so according to Dr. Carl Sagan to obtain -- life!
That is what they go by now, as distance away from a Sun to obtain an Earth-like Planet.
So, unlike the postings -- the best estimate of having life would be that data above about the distance for a Earth-like planet around either of those
2 Suns (stars) there in that System. Yes, I suppose it could be different, but then that is what the astronomers go by for comparing anything in the
Heavens for any Earth-like Planet around any other star up there.
Zeta 2 planet would be looked for at around 82, 491,000 miles from that Sun.
Zeta 1 planet would be looked for at around 93, 930,000 miles from that Sun.
That gives slightly different data than what Anonymous is posting for the distance away for Planet Serpo.
(96 million miles and 91 million miles away).
The Suns are relavtively the same size as our Sun -- (Mass: 1 x Sol)
(Diameter: 0.987 x Sol) for Zeta 2 and (Mass: 0.9 x Sol)
(Diameter: 0.912 x Sol) for Zeta 1.
Sol is our Sun's name!
We compare anything like Planets and Suns to our Solar System.
Source for distance: Hipparcos
Hipparcos is/was a satellite launched back in 1988 or so, and a website is still up for the data that satellite observed.
Any stars up in the sky are in different catalogs and combined as data anyone can look up, and usually kept by NASA with many websites and many
catalogs of data.
[edit on 31-12-2005 by AmoebaSized]