gamma piscium type of starshinedown attention attention
The star used to have the designation 2 Arietis. It is the first star to the east of the Circlet of Pisces.The star is suspected to be a close binary system. situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. The 13th magnitude companion is two arc minutes away and thought to be a K9-class dwarf or merely a star in the same line of sight.Nu Piscium is an orange giant with the stellar classification K3IIIb. It is about 5.4 billion years old, which makes it slightly older than the Sun.54 Piscium is another orange dwarf in Pisces. The time it will take to travel to this star is dependent on how fast you are going. It has an apparent magnitude of 13.9.3C 31 is a double radio galaxy about 237 million light years away in Pisces constellation. Acknowledgment: R. Chandar (University of Toledo) and J. Miller (University of Michigan)M74 has a low surface brightness and of all the Messier objects it is the one most difficult for amateur astronomers to observe. Based on the star's spectral type of G7III , Gamma Piscium's colour and type is yellow giant star. Alpha 1 Piscium ... Fum al Samakah. Unlike most other prominent naked-eye stars, the star Gamma Cassiopeiae does not have a traditional Latin or Arabic name, which is strange considering that the star is relatively bright with a mean apparent magnitude of 2.47, and located right in the center of the distinctive “W” of the constellation Cassiopeia. It has an H II nucleus.NGC 520 is the product of a collision between two disk galaxies that started 300 million years ago. Beta Piscium.
The red dot in the diagram below shows where γ Piscium is situated in One completes an orbit every 7.1 days, while the other one takes eight years to complete an orbit.The astronomer Johannes Hevelius divided Pisces into four subdivisions in his Firmamentum Sobiescianum in 1690: the North Fish (Piscis Boreus), the North Cord (Linum Boreum), the South Cord (Linum Austrinum), and the South Fish (Piscis Austrinus).Piscis Boreus is formed by the stars σ, 68, 65, 67, ψ1, ψ2, ψ3, χ, φ, υ, 91, τ, 82 and 78 Piscium.Piscis Austrinus is formed by the stars ω, ι, θ, 7, β, 5, κ, 9, λ and TX (19) Piscium.Linum Boreum is formed by the stars χ, ρ, 94, VX (97), η, π, ο and α Piscium.Linum Austrinum is formed by the stars α, ξ, ν, μ, ζ, ε, δ, 41, 35 and ω Piscium.Testudo is formed by the stars 24, 27, YY(30), 33 and 29 Piscium.
It has an apparent magnitude of 12.7. γ Piscium is
All stars like planets orbit round a central spot, in the case of planets, its the central star such as the Sun. Lambda Piscium is a main star of the constellation outline. The star belongs to the spectral class G7 IIIa, which means that it is a yellow giant. The figure of 66.47 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.
Young hot stars can, however, be found in small clusters in the outer regions of the galaxy.The Pisces Dwarf was discovered by the Russian astronomer Valentina E. Karachentseva in 1976.Arp 284 is a pair of interacting galaxies in Pisces, discovered by the English astronomer John Herschel in September 1830.NGC 7714 is a spiral galaxy with an apparent magnitude of 12.2, and NGC 7715 is thought to be either an edge-on spiral or an irregular galaxy.A supernova, SN 1999dn, was discovered in NGC 7714 in September 1999.NGC 7714 – Based on observations made with the NASA/ESA Hubble Space Telescope, and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF, ESA) and the Canadian Astronomy Data Centre (CADC, NRC, CSA).NGC 474 is a large elliptical galaxy.
For Gamma Piscium, the location is 23h 17m 09.49 and +03° 16` 56.1 . Gamma Piscium (Gamma Psc, γ Piscium, γ Psc) is a star approximately 138 light years away from Earth, in the zodiac constellation of Pisces.
The constellations that we see today will be different than they were 50,000 years ago or 50,000 years from now. Based on the spectral type (G7III) of the star, the star's colour is yellow.
γ Piscium is Properties.
The companion galaxy, located to the bottom-right of the image, displays an intricate structure, including a number of trails that extend quite far out from its core.
When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Thank you! It is believed to contain about 100 billion stars.The grand-design spiral galaxy Messier 74, image: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA, Hubble Collaboration. moving towards the Sun at the speed of γ Piscium is a giant star
The red arrow shows the motion of γ Piscium during the next
summarizes the key facts about γ Piscium:
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