CK Vulpeculae taken by ALMA.[1] Credit: ALMA (ESO/NAOJ/NRAO)/S. P. S. Eyres
Observation data Epoch J2000.0 Equinox J2000.0
Constellation
Vulpecula
Right ascension
19h 47m 38.0s[2]
Declination
+27° 18′ 48″[2]
Apparent magnitude (V)
max 2.6[2]
Characteristics
B−V color index
0.7[3]
Variable type
unknown[3]
Astrometry
Distance
10000+3000 −2000[4] ly (3200+900 −600[4] pc)
Details
Luminosity
0.9[3]L☉
Temperature
14,000 – 100,000[3] K
Other designations
CK Vulpeculae, CK Vul, Nova Vul 1670, HR 7539, 11 Vul[5]
Database references
SIMBAD
data
CK Vulpeculae (also Nova Vulpeculae 1670) is an object whose exact nature is unknown.[4] It was once considered to be the oldest reliably-documented nova. It consists of a compact central object surrounded by a bipolar nebula.
Models suggest CK Vulpeculae may not be a classic nova; rather it may be classified as a luminous red nova which is the result of two main sequence stars colliding and merging. A 2018 study found it was most likely the result of an unusual collision of a white dwarf and a brown dwarf. A 2020 article ruled out this proposed mechanism and proposes that CK Vulpeculae is an intermediate luminosity optical transient, i.e. an object in the luminosity gap between supernovae and novae.[4]
^"Through the Hourglass". www.eso.org. Retrieved 8 October 2018.
^ abcCite error: The named reference downes was invoked but never defined (see the help page).
^ abcdCite error: The named reference Evans2016 was invoked but never defined (see the help page).
^ abcdCite error: The named reference bane was invoked but never defined (see the help page).
^Morton, Wagman (2003). Lost Stars. Blacksburg, Virginia: McDonald and Woodward. p. 494. ISBN 978-0-939923-78-6.
CKVulpeculae (also Nova Vulpeculae 1670) is an object whose exact nature is unknown. It was once considered to be the oldest reliably-documented nova...
could also exist brown dwarfs that merged with white dwarfs. The nova CKVulpeculae might be a result of such a white dwarf–brown dwarf merger. Substellar...
into his catalog as a star called "34 Tauri". 11 Vulpeculae was a nova, now known as CKVulpeculae. Many of them were caused by arithmetic errors made...
widespread use, it has begun to be applied to some objects like KjPn 8 and CKVulpeculae for which no transient event has been observed, but which may have been...
has already been used to try to explain the mysterious outburst of CKVulpeculae in 1670–1672 that has puzzled scientists for centuries. Past spectroscopic...
star Mira. He is credited with being the first to observe the Nova 1670 Vulpeculae, the first ordinary nova discovered in modern times. In 1681, he published...
identified the post-nova star), with only CKVulpeculae being older. But Naylor et al. argue that CKVulpeculae is not a nova, and WY Sagittae is the oldest...
Harrison, Thomas E. (1996). "A Near-Infrared Survey of Old Novae--II. CKVulpeculae and V605 Aquilae". Publications of the Astronomical Society of the Pacific...
Modelling VLTI/GRAVITY and MATISSE observations of AH Sco, KW Sgr, V602 Car, CK Car and V460 Car". Astronomy & Astrophysics. 683: A19. arXiv:2312.12521. doi:10...