https://br.wikipedia.org/w/index.php?title=Delta_Pavonis&oldid=1472107, an Aotre-Implijout Creative Commons Dereiñ/Kenrannañ diouzh an hevelep divizoù.

Alongside Sol, Tau Ceti, Altair, and Beta Hydri, it was one of the original signatories of the Federal Accord of 2242 and is regarded as a founding member of the Federation.

Delta Pavonis (δ Pav, förkortat Delta Pav, δ Pav) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Påfågeln. Delta Pavonis (88 Pavonis) é uma estrela na direção da constelação de Pavo. Nell'emisfero nord può essere osservata limitatamente durante i mesi estivi dell'emisfero boreale.

Delta Pavonis (δ Pav / HD 190248) è una stella di classe spettrale G5 V-IV, ubicata nella costellazione del Pavone, a quasi 20 anni luce dal sistema solare. Delta Pavonis (δ Pav / δ Pavonis) a zo ur steredenn lec'hiet 19.9 bloavezh-gouloù diouzh an Douar. Ur steredenn c'horre eo, ar pezh a dalvez emañ o vont da baouez da deuziñ hidrojen heg e yelo buanig d'ur ramz ruz.Abalamour d'an dra-se ez eo un tammig skedusoc'h eget an Heol daoust ma'z eo klouaroc'h.. Delta Pavonis er skiant-faltazi. Tuttavia Delta Pavonis sembra essere più antica, con un'età stimata da 6,6 a 6,9 miliardi di anni, e probabilmente sta finendo di fondere l'idrogeno in elio all'interno del suo nucleo evolvendosi in una subgigante, essendo un po' più luminosa di quanto la sua temperatura superficiale lascerebbe pensare. So, in my opinion, if there were any intelligent life supporting planets orbiting δ Pavonis, the all would be dead by now.--JyriL talk 20:33, 13 May 2006 (UTC) Actually, I wouldn't say that Delta Pav is shortly before becoming a red giant.

Tähti saattaa olla kehittymässä alijättiläiseksi. Tähti on spektriluokkaansa nähden kirkas ja siksi "vanha" tähti, joka on kirkastumassa pois pääsarjasta. Delta Pavonis (δ Pav / HD 190248 / HR 7665 / GJ 780)[1] ye la tercera estrella más brillosa na constelación de Pavu, con magnitú aparente +3,55, superada en rellumu por Peacock (α Pavonis) y β Pavonis. La so órbita alredor del centru de la galaxa ye bien similar a la del Sol.[2]. «Astrobiologically interesting stars within 10 parsecs of the Sun». It has been estimated that only in two billion years (or less) the Earth will become inhabitable due to the increased solar luminosity, but even at that time the Sun is still firmly a dwarf star. Si tratta di una stella situata nell'emisfero celeste australe. Il SETI la indica tra i migliori obiettivi tra le 100 stelle di classe G più vicine al Sole, anche se non è stato finora rilevato nessun segnale radio proveniente da tecnologia aliena[5]. Tycho-2 Dwarfs, Old Open Clusters, and the Nearest 100 Stars, Activity indices for southern stars (Jenkins+, 2006), Stellar parameters of nearby cool stars (Takeda+, 2007), Monthly Notices of the Royal Astronomical Society, Stelle principali della costellazione del Pavone, https://it.wikipedia.org/w/index.php?title=Delta_Pavonis&oldid=114936344, licenza Creative Commons Attribuzione-Condividi allo stesso modo.

A questa distanza, esso avrebbe un periodo di circa 413 giorni.

Considerando sua distância de 20 anos-luz em relação à Terra, sua magnitude absoluta é igual a 4.63. It was first colonised between 2190 and 2230. Space: Above and Beyond Wiki is a FANDOM TV Community.

Sua magnitude aparente é igual a 3.55. Parallax measurements from the Hipparcos satellite yield an estimated distance of 19.92 light-years (6.11 parsecs) from Earth.

Sivua on viimeksi muutettu 15. tammikuuta 2018 kello 11.48.

Tähti … Of course it could have had frozen planets waiting for the brightening of the star, but it will be a short time compared to the lifetime of the star when such planets can be habitable making the emergence of life there difficult (not to mention intelligent life).

Delta Pavonis (Delta Pav, δ Pavonis, δ Pav) is a star system located in the Cerberus Sector of the American Arm in the Pavo Constellation.

Delta Pavonis (δ Pav / δ Pavonis) on hyvin aurinkomainen[1] tähti Delta Pavonis is a star in the southern circumpolar constellation of Pavo.

De masa daqué mayor que la masa solar,[3][2] la metalicidá de Delta Pavonis, espresada como la rellación ente los conteníos de fierro ya hidróxenu, ye 2,38 vegaes mayor que la del Sol; yá que esti valor rellacionar cola esistencia de planetes terrestres, especulóse sobre la posibilidá de qu'esistan planetes n'órbita que puedan allugar vida.


Il progetto della NASA Terrestrial Planet Finder, ora posticipato a tempo indefinito, l'aveva indicata come uno dei principali obiettivi di osservazione. Riikinkukon tähtikuviossa eteläisellä tähtitaivaalla, niin etelässä, ettei tähti näy Suomessa. Accurate fundamental parameters for 23 bright solar-type stars, Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics, Target Selection for SETI.

Por ello, anque con una temperatura de 5560 K ye llixeramente más fría que'l Sol, tien una lluminosidá un 18% mayor que la lluminosidá solar.

It has an apparent visual magnitude of 3.56, making it a fourth-magnitude star that is visible to the naked eye from the southern hemisphere.

Coordinate: 20h 08m 43.6s, -66° 10′ 55.4″. Delta Pavonis (δ Pav / δ Pavonis) est une étoile de la constellation du Paon située à 19,9 années-lumière de la Terre. Delta Pavonis (δ Pav / δ Pavonis) a zo ur steredenn lec'hiet 19.9 bloavezh-gouloù diouzh an Douar. Delta Pavonis (δ Pav / δ Pavonis) on hyvin aurinkomainen tähti Riikinkukon tähtikuviossa eteläisellä tähtitaivaalla, niin etelässä, ettei tähti näy Suomessa.

[6], Coordenaes: 20h 8m 43.609s, -66° 10′ 55.443″.

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