The double star ζ Reticuli is located in the western part of the small Reticulum constellation, about 25′ from the constellation's border with Horologium. In dark southern skies, the two stars can be viewed separately with the naked eye, or with a pair of binoculars.[15] ζ1 Reticuli has an apparent magnitude of 5.52,[2] placing it on the border between 5th- and 6th-magnitude stars. ζ2 Reticuli is slightly brighter at magnitude 5.22.[2]
The two stars are located at similar distances from the Sun and share the same motion through space,[16] confirming that they are gravitationally bound and form a wide binary star system. They have an angular separation of 309.2 arcseconds (5.2 arcminutes);[17] far enough apart to appear as a close pair of separate stars to the naked eye under suitable viewing conditions. The distance between the two stars is at least 3,750 AU (0.06 light-year, or almost a hundred times the average distance between Pluto and the Sun), so their orbital period is 170,000 years or more.[18]
Both stars share similar physical characteristics to the Sun,[16] so they are considered solar analogs. Their stellar classification is nearly identical to that of the Sun. ζ1 has 96% of the Sun's mass and 84% of the Sun's radius. ζ2 is slightly larger and more luminous than ζ1, with 99% of the Sun's mass and 88% of the Sun's radius.[19][20] The two stars are somewhat deficient in metals, having only 60% of the proportion of elements other than hydrogen and helium as compared to the Sun.[4][21] For reasons that remain uncertain, ζ1 has an anomalously low abundance of beryllium.[12] Two possible explanations are: during the star's formation it underwent multiple intense bursts of mass accretion from a rapidly rotating protostellar cloud, or else the star underwent rotational mixing brought on by a period of rapid rotation during the star's youth.[22]
Both stars were considered unusual because they were thought to have had a lower luminosity than is normal for main-sequence stars of their age and surface temperature. That is, they lie below the main-sequence curve on the Hertzsprung–Russell diagram for newly formed stars. However, this was challenged, after using the much more accurate parallaxes from the Hipparcos catalogue (ESA, 1997), it was calculated that the stars actually have higher luminosities and so are shifted upwards, putting them in the main sequence.[4] Most stars will evolve above this curve as they age.[17]
ζ1 has an intermediate level of magnetic activity in its chromosphere[23] with an erratic variability. A long-term activity cycle of ~4.2 years has been tentatively identified.[24] ζ2 is more sedate, showing a much lower level of activity[25] with a ~7.9-year cycle, which may indicate it is in a Maunder Minimum state.[24] Although the kinematics of this system suggest that they belong to a population of older stars, the properties of their stellar chromospheres suggests that they are only about 2 billion years old.[26]
This star system belongs to the Zeta Herculis Moving Group of stars that share a common motion through space, suggesting that they have a common origin. In the galactic coordinate system, the [U, V, W] components of the space velocity for this system are equal to [−70.2, −47.4, +16.4] km/s for ζ1 and [−69.7, −46.4, +16.8] km/s for ζ2.[4] They are currently following an orbit through the Milky Waygalaxy that has an eccentricity of 0.24. This orbit will carry the system as close as 17.4 kly (5.335 kpc) and as far as 28.6 kly (8.769 kpc) from the Galactic Center. The inclination of this orbit will carry the stars as much as 1.3 kly (0.4 kpc) from the plane of the galactic disk.[5] This likely puts them outside the thick disk population of stars.[17]
Alleged debris disk
Zeta Reticuli has no known planets. In 2002, ζ1 was examined at an infrared wavelength of 25 μm, but no indication of an excess of infrared radiation was found.[27]
In 2007, the Spitzer Space Telescope was used to find an apparent infrared excess at a wavelength of 70 μm around ζ2. This radiation was attributed to emission by a debris disk with a mean temperature of 150 K (−123 °C), theorized to be orbiting the host star at a distance of 4.3 AU.[28] In 2010, the Herschel Space Observatory, a telescope with a comparatively superior spatial resolution and, unlike Spitzer, able to resolve radiation excesses beyond the wavelength of 70 μm, determined the infrared excess as coming from a two-lobed structure that looked like a debris disk seen edge-on. This debris disk interpreted as an analogy to the Kuiper belt with a semi-major axis of 100 AU and a temperature of 30–40 K.[29]
However, observations with ALMA from October and November 2017 revealed that the structure observed by Herschel shows no common proper motion with Zeta Reticuli. In these observations, no significant flux has been detected around ζ2, showing that the alleged debris disk is not real, but rather a case of background confusion. The observations demonstrate the need to follow up Herschel observations of debris disks.[30]
The 1966 bestseller The Interrupted Journey about Barney and Betty Hill reproduced a "star map" drawn by Betty, allegedly based on one she saw aboard an alien spaceship. Based on the map, a fan of the book named Marjorie Fish speculated that the aliens might originate from Zeta Reticuli. By 1974, the Hill case was referred to as the Zeta Reticuli incident.[31] In a 1980 episode of Cosmos , Carl Sagan demonstrated that the Hill map bore no resemblance to the real-life map.
In the 1988 broadcast UFO Cover Up? Live, alleged government informant "Falcon" (Richard Doty) spread tales of Majestic 12, a hidden cabal that has made a secret treaty with gray aliens from Zeta Reticuli who operate out of Area 51. Alleged Area 51 worker Bob Lazar similarly spread tales of aliens from Zeta Reticuli.
^ abcdefgdel Peloso, E. F.; et al. (June 2000). "zeta1 and zeta2 Reticuli and the existence of the zeta Herculis group". Astronomy and Astrophysics. 358: 233–241. Bibcode:2000A&A...358..233D.
^Evans, D. S. (20–24 June 1966). Batten, Alan Henry; Heard, John Frederick (eds.). "The Revision of the General Catalogue of Radial Velocities". Determination of Radial Velocities and Their Applications, Proceedings from IAU Symposium No. 30. 30. University of Toronto: International Astronomical Union: 57. Bibcode:1967IAUS...30...57E.
^Streicher, Magda (December 2009). "Reticulum: The Celestial Crosshairs". Monthly Notes of the Astronomical Society of South Africa. 68 (11/12): 242–246. Bibcode:2009MNSSA..68..242S.
^ abda Silva, L.; Foy, R. (May 1987). "Zeta-1 and Zeta-2 RETICULI - A puzzling solar-type twin system". Astronomy and Astrophysics. 177 (1–2): 204–216. Bibcode:1987A&A...177..204D.
^Pasinetti Fracassini, L. E.; et al. (February 2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics". Astronomy and Astrophysics. 367 (2): 521–524. arXiv:astro-ph/0012289. Bibcode:2001A&A...367..521P. doi:10.1051/0004-6361:20000451. S2CID425754. Note: using the method of Perrin and Karoji (1987).
^A metallicity of −0.22 indicates that they have the following proportion of metals compared to the Sun: 10−0.22 = 0.603, or 60%.
