Stars Delphinus has two stars above fourth
(apparent) magnitude; its brightest star is of magnitude 3.6. The main
asterism in Delphinus is Job's Coffin, nearly a 45°-apex
lozenge or diamond of the four brightest stars: Alpha, Beta, Gamma, and Delta Delphini. Delphinus is in a rich Milky Way star field. Alpha and Beta Delphini have 19th-century names Sualocin and Rotanev, read backwards: Nicolaus Venator, the Latinized name of a
Palermo Observatory director,
Niccolò Cacciatore (d. 1841).
Alpha Delphini is a blue-white hued
main sequence star of magnitude 3.8, 241 light-years from Earth. It is a spectroscopic binary. It is officially named Sualocin. The star has an absolute magnitude of -0.4.
Beta Delphini is officially called Rotanev. The gap between its close
binary stars is visible from large amateur telescopes. To the unaided eye, it appears to be a white star of magnitude 3.6.
Delta Delphini is a type
A-type star It is a spectroscopic binary, and both stars are
Delta Scuti variables.
Epsilon Delphini, Deneb Dulfim (
lit. "tail [of the] Dolphin"), or Aldulfin, is a star of
stellar class B6 III. Its magnitude is variable at around 4.03.
Zeta Delphini, an A3Va , Delphinus,
Sagitta, and the summer
Milky Way as seen in
Dark-sky preserve Westhavelland Rho Aquilae at magnitude 4.94 Due to its
proper motion, it has been in the (round-figure parameter) bounds of the constellation since 1992. It is an
A-type main sequence star with a lower metallicity than the Sun.
HR Delphini was a
nova that brightened to magnitude 3.5 in December 1967. It took an unusually long time for the nova to reach peak brightness which indicate that it barely satisfied the conditions for a thermonuclear runaway. Another nova by the name
V339 Delphini was detected in 2013; it peaked at magnitude 4.3 and was the first nova observed to produce lithium.
Arion, the planet, is a very dense and massive planet with a mass at least 10.3 times greater than Jupiter. Arion was part of the first
NameExoWorlds contest where the public got the opportunity to suggest names for exoplanets and their host stars.
Exoplanets In 2024 the planet
TOI-6883 b was discovered in the constellation Delphinus. It has a 16.249 day orbital period around its host star, a radius 1.08 times Jupiter's, and a mass 4.34 times Jupiter's. It has an orbital period of 7.8458 days, a radius of 0.7 times Jupiter's, and a third of Jupiter's mass. The Neptunian-size planet was discovered from an abnormality in data retrieved from TOI-6883 c.
Deep-sky objects Its rich
Milky Way star field means many modestly deep-sky objects.
NGC 6891 is a
planetary nebula of magnitude 10.5; another is
NGC 6905 or the Blue Flash Nebula. The Blue Flash Nebula shows broad emission lines. The central star in NGC 6905 has a spectral type of WO2, meaning it is rich in oxygen.
NGC 6934 is a
globular cluster of magnitude 9.75. It is about 52,000 light-years away from the Solar System. It is in the
Shapley-Sawyer Concentration Class VIII and is thought to share a common origin with another globular cluster in
Boötes. It has an intermediate metallicity for a globular cluster, but as of 2018 it has been poorly studied. At a distance of about 137,000 light-years, the globular cluster
NGC 7006 is at the outer reaches of the galaxy. It is also fairly dim at magnitude 11.5 and is in Class I. ==See also==