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Solar analog

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(Redirected from Solar twins) Star that is particularly similar to the Sun "Solar twins" redirects here. For the musical group, see Solar Twins (band). For a star that likely came from the same stellar nursery as the Sun, see Solar sibling.
This illustration compares the somewhat larger and hotter Sun (left) to the relatively inactive star Tau Ceti.

Solar-type stars, solar analogs (also analogues), and solar twins are stars that are particularly similar to the Sun. The stellar classification is a hierarchy with solar twin being most like the Sun followed by solar analog and then solar-type. Observations of these stars are important for understanding better the properties of the Sun in relation to other stars and the habitability of planets.

By similarity to the Sun

Defining the three categories by their similarity to the Sun reflects the evolution of astronomical observational techniques. Originally, solar-type was the closest that similarity to the Sun could be defined. Later, more precise measurement techniques and improved observatories allowed for greater precision of key details like temperature, enabling the creation of a solar analog category for stars that were particularly similar to the Sun. Later still, continued improvements in precision allowed for the creation of a solar-twin category for near-perfect matches.

Similarity to the Sun allows for checking derived quantities—such as temperature, which is derived from the color index—against the Sun, the only star whose temperature is confidently known. For stars that are not similar to the Sun, this cross-checking cannot be done.

Solar-type

These stars are broadly similar to the Sun. They are main-sequence stars with a B−V color between 0.48 and 0.80, the Sun having a B−V color of 0.65. Alternatively, a definition based on spectral type can be used, such as F8V through K2V, which would correspond to B−V color of 0.50 to 1.00. This definition fits approximately 10% of stars, so a list of solar-type stars would be quite extensive.

Solar-type stars show highly correlated behavior between their rotation rates and their chromospheric activity (e.g. Calcium H & K line emission) and coronal activity (e.g. X-ray emission) Because solar-type stars spin down during their main-sequence lifetimes due to magnetic braking, these correlations allow rough ages to be derived. Mamajek & Hillenbrand (2008) have estimated the ages for the 108 solar-type (F8V–K2V) main-sequence stars within 52 light-years (16 parsecs) of the Sun based on their chromospheric activity (as measured via Ca, H, and K emission lines).

The following table shows a sample of solar-type stars within 50 light years that nearly satisfy the criteria for solar analogs (B−V color between 0.48 and 0.80), based on current measurements (the Sun is listed for comparison):

Sample of solar-type stars
Identifier J2000 coordinates Distance
(ly) 		Stellar
class 		Temperature
(K) 		Metallicity
(dex) 		Age
(Gyr) 		Notes
Right ascension Declination
Sun — — 0.0000158 G2V 5778 +0.00 4.6
Rigil Kentaurus  15 49 36.49400 −60° 50′ 02.3737″ 4.37 G2V 5790 +0.20 4.4
Toliman 4.37 K0V 5260 4.4
Epsilon Eridani  -09 27 29.7 03° 32′ 55.8″ 10.4 K2V 5084 -0.13 0.4-0.8
Tau Ceti  01 44 04.1 −15° 56′ 15″ 11.9 G8V 5344 –0.52 5.8
82 Eridani  03 19 55.7 −43° 04′ 11.2″ 19.8 G8V 5338 –0.54 6.1
Delta Pavonis  20 08 43.6 −66° 10′ 55″ 19.9 G8IV 5604 +0.33 ~7
V538 Aurigae  05 41 20.3 +53° 28′ 51.8″ 39.9 K1V 5257 −0.20 3.7
HD 14412  02 18 58.5 −25° 56′ 45″ 41.3 G5V 5432 −0.46 9.6
HR 4587  12 00 44.3 −10° 26′ 45.7″ 42.1 G8IV 5538 +0.18 8.5
HD 172051  18 38 53.4 −21° 03′ 07″ 42.7 G5V 5610 −0.32 4.3
72 Herculis  17 20 39.6 +32° 28′ 04″ 46.9 G0V 5662 −0.37 5
HD 196761  20 40 11.8 −23° 46′ 26″ 46.9 G8V 5415 −0.31 6.6
Nu² Lupi  15 21 48.1 −48° 19′ 03″ 47.5 G4V 5664 −0.34 10.3

Solar analog

These stars are photometrically similar to the Sun, having the following qualities:

  • Temperature within 500 K from that of the Sun (5278 to 6278 K)
  • Metallicity of 50–200% (± 0.3 dex) of that of the Sun, meaning the star's protoplanetary disk would have had similar amounts of dust from which planets could form
  • No close companion (orbital period of ten days or less), because such a companion stimulates stellar activity

Solar analogs not meeting the stricter solar twin criteria include, within 50 light years and in order of increasing distance (The Sun is listed for comparison.):

Identifier J2000 coordinates Distance
(ly) 		Stellar
class 		Temperature
(K) 		Metallicity
(dex) 		Age
(Gyr) 		Notes
Right ascension Declination
Sun — — 0.0000158 G2V 5,778 +0.00 4.6
Sigma Draconis  19 32 21.6 +69° 39′ 40″ 18.8 G9–K0 V 5,297 −0.20 4.7
Beta Canum Venaticorum  12 33 44.5 +41° 21′ 27″ 27.4 G0V 5,930 −0.30 6.0
61 Virginis  13 18 24.3 −18° 18′ 40″ 27.8 G5V 5,558 −0.02 6.3
Zeta Tucanae  00 20 04.3 –64° 52′ 29″ 28.0 F9.5V 5,956 −0.14 2.5
Beta Comae Berenices  13 11 52.4 +27° 52′ 41″ 29.8 G0V 5,970 −0.06 2.0
61 Ursae Majoris  11 41 03.0 +34° 12′ 06″ 31.1 G8V 5,483 −0.12 1.0
HR 511  01 47 44.8 +63° 51′ 09″ 32.8 K0V 5,333 +0.05 3.0
Alpha Mensae  06 10 14.5 –74° 45′ 11″ 33.1 G5V 5,594 +0.10 5.4
HD 69830  08 18 23.9 −12° 37′ 56″ 40.6 K0V 5,410 −0.03 10.6
HD 10307  01 41 47.1 +42° 36′ 48″ 41.2 G1.5V 5,848 −0.05 7.0
HD 147513  16 24 01.3 −39° 11′ 35″ 42.0 G1V 5,858 +0.03 0.4
58 Eridani  04 47 36.3 −16° 56′ 04″ 43.3 G3V 5,868 +0.02 0.6
47 Ursae Majoris  10 59 28.0 +40° 25′ 49″ 45.9 G1V 5,954 +0.06 6.0
Psi Serpentis  15 44 01.8 +02° 30′ 54.6″ 47.8 G5V 5,683 0.04 3.2
HD 84117  09 42 14.4 –23° 54′ 56″ 48.5 F8V 6,167 −0.03 3.1
HD 4391  00 45 45.6 –47° 33′ 07″ 48.6 G3V 5,878 −0.03 1.2
20 Leonis Minoris  10 01 00.7 +31° 55′ 25″ 49.1 G3V 5,741 +0.20 6.5
Nu Phoenicis  01 15 11.1 –45° 31′ 54″ 49.3 F8V 6,140 +0.18 5.7
Helvetios  22 57 28.0 +20° 46′ 08″ 50.9 G2.5IVa 5,804 +0.20 7.0

Solar twin

To date no solar twin that exactly matches the Sun has been found. However, there are some stars that come very close to being identical to the Sun, and are such considered solar twins by members of the astronomical community. An exact solar twin would be a G2V star with a 5,778 K surface temperature, be 4.6 billion years old, with the correct metallicity and a 0.1% solar luminosity variation. Stars with an age of 4.6 billion years are at the most stable state. Proper metallicity, radius, chemical composition, rotation, magnetic activity, and size are also very important to low luminosity variation.

Morgan-Keenan spectral classification of stars. Most common star type in the universe are M-dwarfs, 76%. The Sun is a 4.6 billion year-old G-class (G2V) star and is more massive than 95% of all stars. Only 7.6% are G-class stars

The stars below are more similar to the Sun and having the following qualities:

  • Temperature within 50 K from that of the Sun (5728 to 5828 K) (within 10 K of sun (5768–5788 K)).
  • Metallicity of 89–112% (± 0.05 dex) of that of the Sun, meaning the star's proplyd would have had almost exactly the same amount of dust for planetary formation
  • No stellar companion, because the Sun itself is a solitary star
  • An age within 1 billion years from that of the Sun (3.6 to 5.6 Ga)

Other Sun parameters:

  • Sun rotates on its axis once in about 27 days or 1.997 kilometres (1.241 mi)/s
  • Sun radius is 700,000 kilometres (430,000 mi)
  • Sun chemical composition by mass: hydrogen (73.4%); helium (25%); carbon (0.2%); nitrogen (0.09%);oxygen (0.80%); neon (0.16%); magnesium (0.06%); silicon (0.09&); sulfur (0.05%); iron (0.003%).


The following are the known stars that come closest to satisfying the criteria for a solar twin. The Sun is listed for comparison. Highlighted boxes are out of range for a solar twin. The star may have been noted as solar twin in the past, but are more of a solar analog.

Identifier J2000 coordinates Distance
(ly) 		Stellar
class 		Temperature
(K) 		Metallicity
(dex) 		Age
(Gyr) 		Notes
Right ascension Declination
Sun — — 0.0000158 G2V 5,778 +0.00 4.6
18 Scorpii  16 15 37.3 –08° 22′ 06″ 45.1 G2Va 5,433 −0.03 2.9
HD 150248  16 41 49.8 –45° 22′ 07″ 88 G2 5,750 −0.04 6.2
HD 164595  18 00 38.9 +29° 34′ 19″ 91 G2 5,810 −0.06 4.5
HD 195034  20 28 11.8 +22° 07′ 44″ 92 G5 5,760 −0.04 2.9
HD 117939  13 34 32.6 –38° 54′ 26″ 98 G3 5,730 −0.10 6.1
HD 138573  15 32 43.7 +10° 58′ 06″ 99 G5IV–V 5,757 +0.00 7.1
HD 71334  08 25 49.5 −29° 55′ 50″ 124 G2 5,701 −0.075 8.1
HD 98649  11 20 51.769 –23° 13′ 02″ 135 G4V 5,759 −0.02 2.3
HD 143436  16 00 18.8 +00° 08′ 13″ 141 G0 5,768 +0.00 3.8 (±2.9)
HD 129357  14 41 22.4 +29° 03′ 32″ 154 G2V 5,749 −0.02 8.2
HD 133600  15 05 13.2 +06° 17′ 24″ 171 G0 5,808 +0.02 6.3
HD 186302  19 49 6.43 −70° 11′ 16.7″ 184 G3 5,675 +0.00 4.5
HIP 11915  02 33 49.02 −19° 36′ 42.5″ 190 G5V 5,760 –0.059 4.1
HD 101364  11 40 28.5 +69° 00′ 31″ 208 G5V 5,795 +0.02 7.1
HD 197027  20 41 54.6 –27° 12′ 57″ 250 G3V 5,723 −0.013 8.2
Kepler-452  19 44 00.89 +44° 16′ 39.2″ 1400 G2V 5,757 +0.21 6.0
YBP 1194  08 51 00.8 +11° 48′ 53″ 2934 G5V 5,780 +0.023 ~ 4.2 (± 1.6)

Some other stars are sometimes mentioned as solar-twin candidates such as: Beta Canum Venaticorum; however it has too low metallicities (−0.21) for solar twin. 16 Cygni B is sometimes noted as twin, but is part of a triple star system and is very old for a solar twin at 6.8 Ga. Two solar sibling candidates (similar age, metallicity (−0.113), and kinematics) are Gaia DR2 1927143514955658880 and 1966383465746413568.

By potential habitability

Another way of defining solar twin is as a "habstar"—a star with qualities believed to be particularly hospitable to a life-hosting planet. Qualities considered include variability, mass, age, metallicity, and close companions.

  • At least 0.5–1 billion years old
  • On the main sequence
  • Non-variable
  • Capable of harboring terrestrial planets
  • Support a dynamically stable habitable zone
  • 0–1 non-wide stellar companion stars.

The requirement that the star remain on the main sequence for at least 0.5–1 Ga sets an upper limit of approximately 2.2–3.4 solar masses, corresponding to a hottest spectral type of A0-B7V. Such stars can be 100x as bright as the Sun. Tardigrade-like life (due to the UV flux) could potentially survive on planets orbiting stars as hot as B1V, with a mass of 10 M☉, and a temperature of 25,000 K, a main-sequence lifetime of about 20 million years.

Non-variability is ideally defined as variability of less than 1%, but 3% is the practical limit due to limits in available data. Variation in irradiance in a star's habitable zone due to a companion star with an eccentric orbit is also a concern.

Terrestrial planets in multiple star systems, those containing three or more stars, are not likely to have stable orbits in the long term. Stable orbits in binary systems take one of two forms: S-Type (satellite or circumstellar) orbits around one of the stars, and P-Type (planetary or circumbinary) orbits around the entire binary pair. Eccentric Jupiters may also disrupt the orbits of planets in habitable zones.

Metallicity of at least 40% solar ( = −0.4) is required for the formation of an Earth-like terrestrial planet. High metallicity strongly correlates to the formation of hot Jupiters, but these are not absolute bars to life, as some gas giants end up orbiting within the habitable zone themselves, and could potentially host Earth-like moons.

One example of such a star is HD 70642 , a G5V, at temperature of 5533 K, but is much younger than the Sun, at 1.9 billion years old.

Another such example would be HIP 11915, which has a planetary system containing a Jupiter-like planet orbiting at a similar distance that the planet Jupiter does in the Solar System. To strengthen the similarities, the star is class G5V, has a temperature of 5750 K, has a Sun-like mass and radius, and is only 500 million years younger than the Sun. As such, the habitable zone would extend in the same area as the zone in the Solar System, around 1 AU. This would allow an Earth-like planet to exist around 1 AU.

See also

Footnotes

  1. A true solar twins as noted by the Lowell Observatory should have a temperature within ~10 K of the Sun. Space Telescope Science Institute, Lowell Observatory, noted in 1996 that temperature precision of ~10 K can be measured. A temperature of ~10 K reduces the solar twin list to near zero, so ±50 K is used for the chart.
  2. habstar or habitability, is currently defined as an area, such as a planet or a moon, where liquid water can exist for at least a short duration of time.
  3. The supergiant and following supernova & neutron star (due to >8 M☉ mass) would likely destroy the life at the end of the B1V star's lifetime.

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