
Image of the Trojan asteroids (coloured green) in front of and behind
Jupiter along its orbital path. Also shown is the main asteroid belt between the orbits of
Mars and Jupiter (white) and the
Hilda family of asteroids (brown)
The 'Trojan asteroids' are a large group of objects that share the orbit of the planet
Jupiter around the Sun. Viewed from a coordinate system that is fixed on Jupiter, they appear to orbit one of the two
Lagrangian points of stability, ''L
4'' and ''L
5'', that lie 60° ahead of and behind Jupiter in its orbit. They have
semi-major axes between 5.05
AU and 5.40 AU, and lie in elongated, curved regions around the two Lagrangian points. They are called 'Trojans' because of a convention whereby they are named after characters from the
Trojan War.
The term '
Trojan' is sometimes used to refer to other
small solar system bodies that have similar relationships to other major bodies: for example, there are
Mars Trojans and
Neptune Trojans. The term 'Trojan planets' is used to describe putative planets that have similar orbital relationships with each other and their parent star. However, the term 'Trojan asteroid' by itself refers only to the Jupiter Trojans.
History
E. E. Barnard made the first observation of a Trojan asteroid, in
1904, but the significance of his observation was not noted at the time. Barnard believed he had sighted the recently discovered
Saturnian satellite
Phoebe, which was only two arc-minutes away in the sky at the time, or possibly even a
star. The identity of the point of light Barnard had observed was not realised until an orbit was constructed for the Trojan , an object (re)discovered in
1999. Since he failed to realise what he was looking at, Barnard's observation is now only a historical curiosity.
The first true discovery of a Trojan occurred in February
1906, when the German astronomer
Max Wolf discovered an
asteroid at the L
4 Lagrangian point of the
Sun–
Jupiter system, and named it
588 Achilles. The oddity of its orbit was realized within a few months, and before long, many other asteroids were discovered at this point (and at the other triangular Lagrange point of the Sun–Jupiter system).
As of August
2007, there are 640 numbered Trojan asteroids at L
4 and 536 at L
5, and a further 539 and 509 unnumbered Trojans, respectively.
[1] There are undoubtedly many others too small to be seen with current instruments (in October
1999, a total of 170 had been numbered; by July
2004, that number had grown to 877). The largest of the Trojans is
624 Hektor, measuring 370×195 km.
Nomenclature
Wolf named the first known Trojan after
Achilles, the hero of
Homer's epic poem ''
The Iliad'', which depicts the
Trojan War. Following Wolf's lead, subsequently discovered asteroids in Jupiter's Lagrangian points were given names associated with the ''Iliad'' and the group as a whole were called 'Trojans'. Those in the L
4 point are named after
Greek heroes (the "Greek node" or "Achilles group"), and those at the L
5 point are named after the heroes of
Troy (the "Trojan node"). Confusingly,
617 Patroclus, the first discovered asteroid at the L
5 point, was named before the Greece/Troy rule was devised, and a Greek name thus appears in the Trojan node; the Greek node also has one "misplaced" asteroid,
624 Hektor, named after a Trojan hero. Even more confusingly, the Trojan node is sometimes called the 'Patroclean asteroids' after its most prominent member, even though
Patroclus was Greek.
Originally, the term "Trojan" applied only to asteroids sharing Jupiter's orbit; however, planetoidal bodies have been discovered at the Lagrangian points of
Mars and
Neptune as well, and are also referred to as "Mars Trojans" and "Neptune Trojans" respectively.
Composition
A team from the
Keck Observatory in Hawaii announced in 2006 that they had measured the density of the binary Trojan asteroid
617 Patroclus as being less than that of water ice, suggesting that the pair, and possibly all the Trojan objects, more closely resemble
comets or
Kuiper Belt objects in size and composition—water ice with a layer of dust—than they do the main belt asteroids.
See also
★
List of Trojan asteroids (Greek camp)
★
List of Trojan asteroids (Trojan camp)
★
Pronunciation of Trojan asteroid names
★
List of objects at Lagrangian points
References
1. List of Jupiter Trojans
External links
★
Minor Planet Center's List of Trojan Minor Planets
★
New Trojan asteroid hints at huge Neptunian cloud - New Scientist