Deneb Kaitos (Arabic for "tail of Cetus", also known as Diphda "frog", from the Arabic الضفدع الثاني aD-Dafda‘ aθ-θānī "the second frog") is the common name of β Ceti, the brightest ) is any massive gaseous celestial body in outer space. Stars appear as shining points in the nighttime sky that twinkle because of the effect of the Earths atmosphere and their distance from us. The Sun is an exception: it is the only star sufficiently close to Earth to appear... star in the Orion is a remarkable constellation, visible from most places on the globe (but not always the whole year long). A constellation is a group of stars visibly related to each other in a particular configuration. In three-dimensional space, most of the stars we see have little relation to one... constellation Cetus (a name from Greek mythology, referring to a Whale or Sea Monster) is a constellation of the southern sky, in the region known as the Water, near other watery constellations like Aquarius, Pisces, and Eridanus. Notable features This constellations most notable star is Mira (ο Ceti), the first... Cetus. Deneb Kaitos is easy to locate due to its location in an otherwise dark corner of the sky.

Deneb Kaitos has a In astronomy, stellar classification is a classification of stars based initially on photospheric temperature and its associated spectral characteristics, and subsequenly refined in terms of other characteristics. Stellar temperatures can be classified by using Wiens displacement law; but this poses difficulties for distant stars. Stellar spectroscopy offers a way... spectral type falling on the border between G and K, making it a yellowish-orange star somewhat cooler than the The Sun (occasionally referred to as Current SOHO snapshots Far-Side Helioseismic Holography from Stanford NASA Eclipse homepage Nasa SOHO (Solar & Heliospheric Observatory) satelliteFAQ Solar Sounds from Stanford Spaceweather.com Eric Weissteins World of Astronomy - Sun Categories: Sun | Main sequence stars ... Sun. In spite of its cooler nature, Deneb Kaitos is several times brighter than the Sun due to it being more massive and having several times the Sun's The word radius of a circle or sphere is the length of any such segment. More generally — in geometry, engineering, graph theory, and many other contexts — the radius of something (e.g. a cylinder, a graph, or a mechanical part) is the distance from its center or axis... radius, as Deneb Kaitos appears to be an older star leaving the Hertzsprung-Russell diagram The main sequence of the Hertzsprung-Russell diagram is the curve where the majority of stars are located in this diagram. Stars located on this band are known as main-sequence stars or dwarf stars. The coolest dwarfs are the red dwarfs. This line is so pronounced... main sequence on its way through the According to the Hertzsprung-Russell diagram, a red giant is a large non-main sequence star of stellar classification K or M; so-named because of the reddish appearance of the cooler giants. Examples include Aldebaran and Arcturus. They are believed to be stars of solar mass or higher which... red giant phase of its In astronomy, stellar evolution is the sequence of changes that a star undergoes during its lifetime, the millions or billions of years during which it emits light and heat. Over the course of that time, the star will change radically. Stellar evolution is not studied by observing the life cycle... evolution. With an The apparent magnitude (, of a star or galaxy is the apparent magnitude it would have if it were 10 parsecs away; that of a planet (or other solar system body) is the apparent magnitude it would have if it were 1 astronomical unit away from both the Sun and Earth... apparent magnitude of 2.04 it ranks among the brighter stars in our night sky, and an In astronomy, absolute magnitude is the apparent magnitude, ) In stellar and galactic astronomy, the standard distance is 10 parsecs (about 32.616 light years, or 1014 kilometres). A star at ten parsecs has a parallax of 0.1 (100 milli arc seconds). In defining absolute magnitude it is necessary to... absolute magnitude of -0.31. At only 96 A light year, abbreviated ly, is the distance light travels in one year: roughly 9.46   1012 kilometres (9.46 petametres, or about 5.88   1012 miles). More specifically, a light year is defined as the distance that a photon would travel, in free space and... light years from the Earth, also known as the Earth or Terra, is the third planet outward from the Sun. It is the largest of the solar systems terrestrial planets, and the only planetary body that modern science confirms as harboring life. The planet formed around 4.5 billion (4.5×109) years... Earth, Deneb Kaitos is one of the nearer stars of a bright apparent magnitude. It can be located at In astronomy declination (dec) is one of the two coordinates of the equatorial coordinate system, the other being either right ascension or hour angle. Dec is comparable to latitude, projected unto the celestial sphere, and is measured in degrees north of the celestial equator. Therefore, points north of the celestial... declination -17° 59' 11.81" and Right ascension (RA; symbol α: Greek letter alpha) is the astronomical term for one of the two coordinates of a point on the celestial sphere when using the equatorial coordinate system. The other coordinate is the declination. RA is comparable to longitude, measured from a zero point known as the... right ascension of 00:43:35.23 (2000).