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Star in the constellation Scutum
Zeta Scuti, Latinized from ζ Scuti, is the Bayer designation for a star in the southern constellation of Scutum. It is a faint star but visible to the
Zeta_Scuti
Star system in the constellation Boötes
F-type main-sequence star. It is a Delta Scuti variable with a brightness amplitude of 0.00134 magnitudes. Zeta Bootis imaged with the Nordic Optical Telescope
Zeta_Boötis
Star in the constellation Ursa Minor
variability was suspected by R. A. Baker in 1926, and it may be a Delta Scuti variable. It is a pulsating variable star, with a period of 15.8 hours,
Zeta_Ursae_Minoris
exoplanets. 83 Aquarii (h Aquarii) A 209 ± 8 Aquarius F2Vn 5.43 B F2V Zeta Scuti 210 ± 10 Scutum G9 IIIb Fe-0.5 4.66 HD 108236 210.6 ± 0.2 G5V 9.24 Has
List of star systems within 200–250 light-years
List_of_star_systems_within_200–250_light-years
Pattern of stars recognized on Earth's night sky
consists of the stars 14, 15, Lambda and 12 Aquilae, Eta Scuti, HD 174208, R and Beta Scuti. The compact open cluster Messier 11 is also aligned with
Asterism_(astronomy)
Constellation in the southern celestial hemisphere
known planet approximately 20.13 parsecs (65.7 ly) away; X Caeli, a Delta Scuti variable that forms an optical double with γ1 Caeli; and HE0450-2958, a
Caelum
Constellation in the northern celestial hemisphere
Retrieved 13 January 2013. Templeton, Matthew (16 July 2010). "Delta Scuti and the Delta Scuti Variables". Variable Star of the Season. AAVSO (American Association
Canis_Minor
Constellation in the southern celestial hemisphere
Retrieved 2 February 2014. Templeton, Matthew (16 July 2010). "Delta Scuti and the Delta Scuti Variables". Variable Star of the Season. AAVSO (American Association
Tucana
Constellation in the northern celestial hemisphere
Retrieved 8 August 2018. Templeton, Matthew (16 July 2010). "Delta Scuti and the Delta Scuti Variables". Variable Star of the Season. AAVSO (American Association
Pegasus_(constellation)
Constellation in the northern celestial hemisphere
pulsate as Delta Scuti-type stars. The distinction between the Lambda Boötis stars as a class of stars with peculiar spectra, and the Delta Scuti stars whose
Boötes
Constellation in the northern celestial hemisphere
Retrieved 18 May 2014. Templeton, Matthew (16 July 2010). "Delta Scuti and the Delta Scuti Variables". Variable Star of the Season. AAVSO (American Association
Ursa_Minor
Constellation in the northern celestial hemisphere
magnitude 4.43. It is a spectroscopic binary, and both stars are Delta Scuti variables. Epsilon Delphini, Deneb Dulfim (lit. "tail [of the] Dolphin")
Delphinus
Minor constellation in the southern sky
1071/AS06025. S2CID 122809222. Templeton, Matthew (16 July 2010). "Delta Scuti and the Delta Scuti Variables". Variable Star of the Season. AAVSO (American Association
Phoenix_(constellation)
Constellation in the northern celestial hemisphere
main-sequence star of spectral type A0Va. Only 7.7 parsecs distant, Vega is a Delta Scuti variable, varying between magnitudes −0.02 and 0.07 over 0.2 days. On average
Lyra
Constellation split into two non-contiguous parts
provide nearly all the light. The primary, a white subgiant, is a Delta Scuti variable with an average apparent magnitude of 4.23. Positioned very near
Serpens
May 22, 2026. "Samurai Jay presenta il nuovo album Amatore su Radio Zeta". Radio Zeta (in Italian). Retrieved May 22, 2026. Serna, Ana (May 22, 2026). "Neutro
2026_in_hip-hop
Star in the constellation Ursa Minor
and Kochab (the full name Ahfa al Farkadain is traditionally applied to Zeta Ursae Minoris). Gamma Ursae Minoris was mostly called Pherkad Major to distinguish
Pherkad
± 9 Aquarius K5 III +4.042 W Hydrae 319 Hydra M7.5e-M9 7.7 - 11.6 Gamma Scuti 319 ± 8 Scutum A2:V 4.67 108 Aquarii (i³ Aquarii) 319 ± 10 Aquarius A0VpSiSr
List of star systems within 300–350 light-years
List_of_star_systems_within_300–350_light-years
Constellation in the Southern Celestial Hemisphere
it is around 5819 times as luminous as the Sun. BF Antliae is a Delta Scuti variable that varies by 0.01 of a magnitude. HR 4049, also known as AG Antliae
Antlia
Constellation in the Southern Celestial Hemisphere
x. S2CID 15358380. Templeton, Matthew (16 July 2010). "Delta Scuti and the Delta Scuti Variables". Variable Star of the Season. American Association
Corvus_(constellation)
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
Scuti V452 Scuti, LBV candidate V1429 Aquilae (= MWC 314), LBV candidate with a supergiant companion. V1768 Cygni V2140 Cygni V4030 Sagittarii Zeta¹
Hypergiant
Catanzarite, J.; Conrow, T.; Laher, R. (2005-02-01). "Altair: The Brightest δ Scuti Star". The Astrophysical Journal. 619 (2): 1072–1076. arXiv:astro-ph/0405127
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Constellation in the southern celestial hemisphere
days. AI Velorum is located 2.8 degrees north-northeast of Gamma, a Delta Scuti variable of spectral type A2p-F2pIV/V that ranges between magnitudes 6.15
Vela_(constellation)
Type of variable star that pulsates radially
evolutionary histories: classical Cepheids and type II Cepheids. Delta Scuti variables are A-type stars on or near the main sequence at the lower end
Cepheid_variable
Constellation in the northern celestial hemisphere
the Sun and Neptune. The brighter component has been classed as a Delta Scuti variable star, though this view is not universal. The components are main
Corona_Borealis
Stars with a supergiant luminosity class with a spectral type of K or M
hypergiants: Stephenson 2 DFK 1 Mu Cephei VV Cephei A NML Cygni S Persei UY Scuti VY Canis Majoris Westerlund 1 W26 WOH G64 A KY Cygni BI Cygni VX Sagittarii
Red_supergiant
star(s) held the title of brightest star during this period. This is due to Zeta Sagittarii, the titleholder on Tomkin's list, being revealed to have been
Historical_brightest_stars
Constellation in the northern celestial hemisphere
equatorial bulge that is 24% larger than the polar radius. It is a Delta Scuti variable with a small amplitude and period of 2.5 hours. Gamma Cassiopeiae
Cassiopeia_(constellation)
Stars in system Spectral type Apparent magnitude (V) Comments and references Zeta Ophiuchi 440 ± 40 1 O9.5 V 2.56 – 2.58 The closest O-type star to Earth.
List_of_O-type_stars
French astrophysicist (1902–1996)
(with Daniel Chalonge and Vladimir Kurganoff) (1949) The spectrum of Nova Scuti (with Vladimir Kurganoff and G. Munch) (1949) Occultations observed at Renée
Renée_Canavaggia
3.72 Delta Virginis (Minelauva) 198 ± 3 Virgo M3+ III 3.32 - 3.40 Alpha Scuti (Tianbian) 199 ± 3 Scutum K3III 3.83 System Star or (sub-) brown dwarf Distance
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
Second brightest star in the southern constellation of Pictor
and one at 36.9 minutes. As a result, the star is classified as a Delta Scuti variable. The mass of Beta Pictoris has been determined from the orbital
Beta_Pictoris
Type of variable star
; Mróz, M. (2023). "The OGLE Collection of Variable Stars. Over 15000 δ Scuti Stars in the Large Magellanic Cloud". Acta Astronomica. 73 (2): 105–126
Classical_Cepheid_variable
binary evolution to the Wolf-Rayet phase: Keck and HST proper motions of RY Scuti's nebula". Monthly Notices of the Royal Astronomical Society. 418 (3): 1959–1972
List_of_supernova_candidates
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