Gamma Cephei Ab (abbreviated γ Cephei Ab, γ Cep Ab), formally named Tadmor , is an
exoplanet
An exoplanet or extrasolar planet is a planet outside the Solar System. The first confirmed detection of an exoplanet was in 1992 around a pulsar, and the first detection around a main-sequence star was in 1995. A different planet, first det ...
approximately 45
light-years away in the
constellation
A constellation is an area on the celestial sphere in which a group of visible stars forms Asterism (astronomy), a perceived pattern or outline, typically representing an animal, mythological subject, or inanimate object.
The first constellati ...
of
Cepheus that orbits
Gamma Cephei A. The planet was suspected to exist in 1988, and later confirmed in 2003, technically making it the first exoplanet discovered.
Naming
In July 2014 the
International Astronomical Union (IAU) launched
NameExoWorlds, a process for giving proper names to certain exoplanets. The process involved public nomination and voting for the new names. In December 2015, the IAU announced the winning name for this planet was Tadmor. It was submitted by the
Syria
Syria, officially the Syrian Arab Republic, is a country in West Asia located in the Eastern Mediterranean and the Levant. It borders the Mediterranean Sea to the west, Turkey to Syria–Turkey border, the north, Iraq to Iraq–Syria border, t ...
n Astronomical Association and is the ancient
Semitic name and modern
Arabic
Arabic (, , or , ) is a Central Semitic languages, Central Semitic language of the Afroasiatic languages, Afroasiatic language family spoken primarily in the Arab world. The International Organization for Standardization (ISO) assigns lang ...
name for the city of
Palmyra, a (
UNESCO
The United Nations Educational, Scientific and Cultural Organization (UNESCO ) is a List of specialized agencies of the United Nations, specialized agency of the United Nations (UN) with the aim of promoting world peace and International secur ...
)
World Heritage Site.
Detection and discovery
1988 claims
The first indications of γ Cephei Ab were reported in July 1988. The planet was tentatively identified by a
Canadian team of astronomers, which was led by
Bruce Campbell,
Gordon Walker and
Stephenson Yang, while its existence was also announced by
Anthony Lawton and P. Wright in 1989. Though not confirmed, this would have been the first ''true'' discovery of an
extrasolar planet, and it was hypothesized based on the same
radial velocity technique later used successfully by others. However, the claim was retracted in 1992 due to the quality of the data not being good enough to make a solid discovery.
2003 confirmation
On 7 May 2003, γ Cephei Ab was finally confirmed. The team of astronomers (including
William D. Cochran,
Artie P. Hatzes, et al.) at the Planetary Systems and their Formation Workshop announced the preliminary confirmation of a long-suspected planet γ Cephei Ab with a minimum mass of 1.59 M
J (1.59 times that of
Jupiter
Jupiter is the fifth planet from the Sun and the List of Solar System objects by size, largest in the Solar System. It is a gas giant with a Jupiter mass, mass more than 2.5 times that of all the other planets in the Solar System combined a ...
).
The parameters were later recalculated when direct detection of the secondary
star
A star is a luminous spheroid of plasma (physics), plasma held together by Self-gravitation, self-gravity. The List of nearest stars and brown dwarfs, nearest star to Earth is the Sun. Many other stars are visible to the naked eye at night sk ...
γ Cephei B allowed astronomers to better constrain the properties of the system.
γ Cephei Ab moves in an elliptical orbit with a
semimajor axis of 2.044 AU which takes almost two and a half years to complete. The eccentricity is 0.115, which means it moves between 1.81 and 2.28 AU in orbital distance around
γ Cephei A, which would place it from slightly beyond the orbit of
Mars to the inner
asteroid belt in the
Solar System
The Solar SystemCapitalization of the name varies. The International Astronomical Union, the authoritative body regarding astronomical nomenclature, specifies capitalizing the names of all individual astronomical objects but uses mixed "Sola ...
.
Astrometric observations
''
Hipparcos'' data taken in 2006 constrains its mass below "13.3 M
J at the 95% confidence level, and 16.9 M
J at the 99.73% (3 σ) confidence level". This is not much to go on, but it is enough to verify that it is not another unseen
brown or
red dwarf.
In 2018,
Hubble astrometric observations revealed the true mass of γ Cephei Ab to be 9.4 .
See also
*
Dimidium
*
HD 114762 b
*
Iota Horologii b
*
Poltergeist
*
Phobetor
References
External links
*
*
{{DEFAULTSORT:Gamma Cephei Ab
Gamma Cephei
Exoplanets discovered in 1988
Giant planets
Exoplanets with proper names
Exoplanets detected by radial velocity
Exoplanets detected by astrometry