V1400 Centauri (1SWASP J140747.93-394542.6) – gwiazda w gwiazdozbiorze Centaura, położona w odległości około 454 lat świetlnych od Słońca.Orbituje wokół niej przynajmniej jeden obiekt, przypuszczalnie planeta otoczona przez olbrzymie pierścienie planetarne
V1400 Centauri Dari Wikipedia bahasa Indonesia, ensiklopedia bebas 1SWASP J140747.93-394542.6 (sering disingkat 1SWASP J140747 atau J1407) adalah sebuah bintang mirip Matahari yang terletak di rasi bintang Centaurus, berjarak sekitar 420 tahun cahaya dari Bumi.
In 2007, J1407 was observed to be eclipsed and orbited by at least one major body, 1SWASP J1407b (J1407b), thought to be either a large gas giant planet or a brown dwarf with an immense ring system. V1400 Centauri / V1400 Cen is recognised by SIMBAD, the American Association of Variable Star Observers, and at least two scientific papers, as the variable star designation for this system. V1400 Centauri From Wikipedia the free encyclopedia. 1SWASP J140747.93−394542.6 ; A graph of 1SWASP J1407 and J1407b to scale, showing the extent of the J1407b orbits its parent star, 1SWASP J140747.93−394542.6 (known simply as V1400 Centauri) in an eccentric (oval) orbit, which could disrupt J1407b's own ring system.
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The star is variable due to the planet orbiting around it and has been given the variable star designation V1400 Centauri. In 2007, J1407 was observed to be eclipsed and orbited by at least one major body, 1SWASP J1407b (J1407b), thought to be either a large gas giant planet or a brown dwarf with an immense ring system.
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In 2007, J1407 was observed to be eclipsed and orbited by at least one major body, 1SWASP J1407b (J1407b), thought to be either a large gas giant planet or a brown dwarf with an immense ring system. V1400 Centauri / V1400 Cen is recognised by SIMBAD, the American Association of Variable Star Observers, and at least two scientific papers, as the variable star designation for this system. V1400 Centauri From Wikipedia the free encyclopedia. 1SWASP J140747.93−394542.6 ; A graph of 1SWASP J1407 and J1407b to scale, showing the extent of the J1407b orbits its parent star, 1SWASP J140747.93−394542.6 (known simply as V1400 Centauri) in an eccentric (oval) orbit, which could disrupt J1407b's own ring system.
Gas Giants are the largest and most perplexing type of planet. From their intensely pressurised cores to their beautiful outer atmospheres- in the Solar System, there are four: Jupiter, Saturn, Uranus & Neptune. in this episode of #OOTW, we will be visiting each of the four giants in the Solar System, before venturing out to see what's in space.
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Extreme edge H~3 emission gives V= 1400.
The star is variable due to the planet orbiting around it and has been given the variable star designation V1400 Centauri. J1407 (V1400 Centauri) is a star 434 light years from Sun and is the parent to J1407b. V1400 Centauri (Q9130002) From Wikidata. Jump to navigation Jump to search.
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English: A to-scale graph of 1SWASP J14 07 47.93 -39 45 42.6 and b to scale. In this image, 1 pixel is 0.01 AU. The sizes of 1SWASP J1407 and 1SWASP J1407b are about 0.0095 AU and 0.007 AU, so rounded up they occupy a single pixel.