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Although designated 'beta', it is actually brighter than the 'alpha' star in the constellation (Alpha Ceti). This orange giant is easy to identify due to its location in an otherwise dark section of the celestial sphere. 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class="text-muted"> An Entity of Type: <a href="http://dbpedia.org/ontology/Star">star</a>, from Named Graph: <a href="http://dbpedia.org">http://dbpedia.org</a>, within Data Space: <a href="http://dbpedia.org">dbpedia.org</a> </div> </div> </div> <div class="row pt-2"> <div class="col-xs-9 col-sm-10"> Beta Ceti (β Ceti, abbreviated Beta Cet, β Cet), officially named Diphda /ˈdɪfdə/, is the brightest star in the constellation of Cetus. Although designated 'beta', it is actually brighter than the 'alpha' star in the constellation (Alpha Ceti). This orange giant is easy to identify due to its location in an otherwise dark section of the celestial sphere. Based on parallax measurements, it lies at an estimated distance of 96.3 light-years (29.5 parsecs) from the Sun. </div> <div class="col-xs-3 col-sm-2"> <a href="#" class="thumbnail"> <img src="http://commons.wikimedia.org/wiki/Special:FilePath/Cetus_constellation_map.svg?width=300" alt="thumbnail" class="img-fluid" /> </a> </div> </div> </div> </section>   <section> <div class="container-xl"> <div class="row"> <div class="table-responsive"> <table class="table table-hover table-sm table-light"> <thead> <tr> <th class="col-xs-3 ">Property</th> <th class="col-xs-9 px-3">Value</th> </tr> </thead> <tbody> <tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/ontology/abstract">dbo:abstract</a> </td><td class="col-10 text-break"><ul> <li style="display:none;">أو بيتا القيطس Beta Ceti اسمه التقليدي Diphda مشتق من الاسم العربي وهو نجم في كوكبة القيطس. ينتمي إلى الفئة الطيفية بين G وK وبالتالي هو نجم مصفر ابرد نوعا ما من الشمس وعلى الرغم من ذلك فهو أكثر ضياء من الشمس وتبلغ كتلته 3 أضعاف كتلة الشمس ونصف قطره حوالي 17 ضعف من نصف قطر الشمس. وهذا النجم انهى مرحلة النسق الأساسي وفي طريقه للتطور إلى مرحلة عملاق أحمر. يبلغ قدره الظاهري 2.04 ويبعد 96 سنة ضوئية عن الأرض اما الضفدع الثاني فيسمى أيضا فم الحوت. (ar)</li> <li style="display:none;">Diphda (Beta de la Balena / β Ceti) és l'estel més brillant de la constel·lació de la Balena. Ocasionalment és superada per la variable Mira (ο Ceti), quan aquesta aconsegueix la seva màxima lluentor. De magnitud aparent de +2,04, és fàcil de localitzar en estar situada en una zona fosca del cel. A la Xina era coneguda com a Too Sze Kung, «el superintendent de les excavacions (edificacions)». (ca)</li> <li style="display:none;">Deneb Kaitos (Beta Ceti, β Cet) je nejjasnější hvězda v souhvězdí Velryby. Přestože je označena „beta“, je ve skutečnosti jasnější než . Jedná se o obra spektrální třídy K0. Lze jej snadno nalézt, neboť v jeho blízkosti nejsou žádné jiné jasné hvězdy. Měřením paralaxy byla zjištěna vzdálenost kolem 96,4 světelných let (29,6 parseků). (cs)</li> <li style="display:none;">Deneb Kaitos (arab. Schwanz des Ungeheuers) ist die Bezeichnung des Sterns β Ceti (Beta Ceti). Deneb Kaitos hat eine scheinbare Helligkeit von 2,04 mag und ist damit (trotz seiner Bezeichnung) heller als α Ceti und hellster Stern im Sternbild Walfisch. Er ist ein Oranger Riese (Red Clump Star) vom Spektraltyp K0 in einer Entfernung von knapp 100 Lichtjahren (Hipparcos Datenbank).Deneb Kaitos wird manchmal auch Diphda (Frosch) genannt. Andere Namen: Difda al Thani von الضفدع الثاني aḍ-ḍafdaʿ aṯ-ṯānī ‚der zweite Frosch‘ („der erste Frosch“ ist Fomalhaut), sowie gleichbedeutend Rana Secunda. Die IAU hat am 21. August 2016 den Eigennamen Diphda als standardisierten Eigennamen für diesen Stern festgelegt. (de)</li> <li>Beta Ceti (β Ceti, abbreviated Beta Cet, β Cet), officially named Diphda /ˈdɪfdə/, is the brightest star in the constellation of Cetus. Although designated 'beta', it is actually brighter than the 'alpha' star in the constellation (Alpha Ceti). This orange giant is easy to identify due to its location in an otherwise dark section of the celestial sphere. Based on parallax measurements, it lies at an estimated distance of 96.3 light-years (29.5 parsecs) from the Sun. (en)</li> <li style="display:none;">Deneb Kaitos (β Ceti / 16 Ceti / HD 4128 / HR 188 / HIP 3419) es la estrella más brillante de la constelación de Cetus, la ballena. Ocasionalmente es superada por la variable Mira (ο Ceti), cuando ésta alcanza su máximo brillo.De magnitud aparente de +2,04, es fácil de localizar al estar situada en una zona oscura del cielo. (es)</li> <li style="display:none;">Beta Ceti (β Cet / β Ceti), également appelée par ses noms traditionnels Diphda et Deneb Kaitos, est l'étoile la plus brillante de la constellation de la Baleine. En dépit de sa désignation de Bayer « beta », elle est en réalité plus brillante que Alpha Ceti. Il s'agit d'une étoile géante orangée plus grande et plus lumineuse que le Soleil, qui est de type spectral G9.5 III ou K0 III et qui est donc à la limite entre les étoiles de type G et de type K. (fr)</li> <li style="display:none;">Beta Ceti (β Cet / β Ceti) adalah bintang paling terang di rasi Cetus. Bintang ini mempunyai klasifikasi antara G dan K, membuat bintang ini dirujukkan sebagai bintang yang hampir sama dengan Matahari. Meskipun demikian, bintang ini lebih cemerlang dan lebih besar daripada Matahari. Beta Ceti adalah bintang yang cukup tua dan mendekati tahapan bintang raksasa merah. Dengan magnitudo sebesar 2.04 membuat bintang ini termasuk bintang yang cemerlang di langit malam. Bintang ini berada pada jarak 96 tahun cahaya dari Bumi. (in)</li> <li style="display:none;">くじら座β星は、くじら座の恒星で2等星。 (ja)</li> <li style="display:none;">데네브 카이토스(Deneb Kaitos)는 고래자리에서 가장 밝은 별로, 지구에서 약 96광년 떨어져 있다. 바이어 명명법에 의하면 고래자리 베타이다. 베타임에도 불구하고, 데네브 카이토스는 알파별인 멘카르보다 더 밝다. 고유 명칭은 디프다(Diphda)라고 한다. 데네브 카이토스 주변은 상대적으로 어둡기 때문에 찾기가 쉽다. (ko)</li> <li style="display:none;">Deneb Kaitos (beta Ceti) is de helderste ster in het sterrenbeeld Walvis (Cetus). De naam is afkomstig uit het Arabisch en staat voor staart van de Walvis. Het Arabische Kaitos is een variant van het Latijnse Cetus.Deneb zonder meer is een andere ster, de staart van de Zwaan. De ster staat ook bekend als Diphda, Difda, Difda al Thani en Rana Secunda. De laatste naam is Spaans en betekent "tweede kikker", de eerste kikker is de ster Fomalhaut in het sterrenbeeld Zuidervis. Deneb Kaitos is een felle reus een hete corona met een massa van drie zonnemassa's welke ongeveer 20.000 keer meer röntgenstraling uitstraalt dan de Zon. Astronomen vermoeden dat dit veroorzaakt wordt doordat de ster zich in een vergevorderd stadium van heliumverbranding bevindt. In dit stadium is de kern van de ster zeer heet (meer dan honderd miljoen graden Celsius) waarbij helium door middel van kernfusie in koolstof omgezet wordt. Met kennis over de sterevolutie is het mogelijk om een beeld te krijgen van de levensloop van Deneb Kaitos. De ster hield zich de eerste miljard jaar van zijn bestaan bezig met het verbranden van waterstof tot helium. Nadat het helium in de kern was uitgeput trok het midden van de ster samen totdat waterstofgas rond de heliumkern heet en dicht genoeg werd om hier kernfusiereacties te laten ontsteken. Deze krachtige nieuwe energiebron deed de buitenste delen van de ster sterk uitzetten en afkoelen. Gedurende deze periode werd Deneb Kaitos een rode reus. Na ongeveer 10 miljoen jaar trok de kern van de ster samen en warmde op tot zo'n 100 miljoen graden zodat heliumfusie plaats kon vinden. In dit stadium, dat 100 miljoen jaar of langer kan duren, is de diameter van de ster geslonken tot 20 keer die van onze zon en is de oppervlaktetemperatuur gestegen zodat het geen rode reus meer is. (nl)</li> <li style="display:none;">Deneb Kaitos (β Cet / β Ceti / Beta Ceti), conosciuta anche come Diphda) è la stella più luminosa della costellazione della Balena, nonostante Bayer le abbia assegnato la lettera β. Il suo nome proprio deriva dall'arabo e significa coda della Balena, mentre il nome alternativo Diphda deriva sempre dall'arabo الضفدع الثاني, al-ḍafdaʿ al-thānī, che significa la seconda rana (essendo invece la prima Fomalhaut). (it)</li> <li style="display:none;">Diphda (Beta Ceti, Deneb Kaitos) – najjaśniejsza gwiazda w gwiazdozbiorze Wieloryba (wielkość gwiazdowa: 2,01m). Odległa od Słońca o około 96 lat świetlnych. (pl)</li> <li style="display:none;">Deneb Kaitos – Diphda, eller Beta Ceti (β Ceti, förkortat Beta Cet, β Cet), som är stjärnans Bayer-beteckning, är en ensam stjärna i sydvästra delen av stjärnbilden Valfisken. Den har en skenbar magnitud av 2,02, är den ljusaste stjärnan i stjärnbilden trots att dess Bayer-beteckning tyder på att den skulle vara näst starkast, och är synlig för blotta ögat. Baserat på parallaxmätningar i Hipparcos-uppdraget på 33,9 mas beräknas den befinna sig på ca 96 ljusårs (30 parsek) avstånd från solen. (sv)</li> <li style="display:none;">Beta Ceti (Deneb Kaitos, Diphda, Difda al Thani, Rana Secunda, 16 Ceti) é uma estrela na direção da Cetus. Possui uma ascensão reta de 00h 43m 35.23s e uma declinação de −17° 59′ 12.1″. Sua magnitude aparente é igual a 2.04. Considerando sua distância de 96 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.30. Pertence à classe espectral K0III. É uma estrela variável suspeita. (pt)</li> <li style="display:none;">Бета Кита — ярчайшая звезда созвездия Кита. Имеет традиционные названия Дифда и Денеб Кайтос. Бета Кита является оранжевым гигантом спектрального класса K0III. Это — старая звезда, которая вступает в финальный этап своего жизненного цикла. Имея массу в 3 массы Солнца, Бета Кита ярче Солнца (болометрически, то есть по всем длинам волн вместе) в 145 раз и в 17 раз больше по диаметру. Температура поверхности звезды составляет около 4500 °C. Расстояние до Земли — 96 световых лет. Видимая звёздная величина +2.04. Как и Сириус, Бета Кита уверенно доступна для наблюдения в Европе. Наблюдается южнее 72 градусов северной широты. Низко поднимается над горизонтом на широтах Мурманска, Норильска и Воркуты. Южнее 72 градусов южной широты звезда не заходит за горизонт. (ru)</li> <li style="display:none;">土司空（英語：Diphda），也称为鯨魚座β（beta Ceti、简写β Cet）。是鲸鱼座最亮的恒星，视星等为2.02等，绝对星等为−0.31等。土司空位於夜空中的陰暗角落，所以人們可以很容易的觀察到它的位置。因為它距離地球僅96.3光年，所以土司空是距離最近的明亮恆星之一。 (zh)</li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://dbpedia.org/ontology/thumbnail">dbo:thumbnail</a> </td><td class="col-10 text-break"><ul> <li><a class="uri" rel="dbo:thumbnail" resource="http://commons.wikimedia.org/wiki/Special:FilePath/Cetus_constellation_map.svg?width=300" href="http://commons.wikimedia.org/wiki/Special:FilePath/Cetus_constellation_map.svg?width=300">wiki-commons:Special:FilePath/Cetus_constellation_map.svg?width=300</a></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/ontology/wikiPageExternalLink">dbo:wikiPageExternalLink</a> </td><td class="col-10 text-break"><ul> <li><a class="uri" rel="dbo:wikiPageExternalLink nofollow" resource="http://chandra.harvard.edu/photo/2004/bceti/" 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href="http://www.w3.org/2000/01/rdf-schema#comment">rdfs:comment</a> </td><td class="col-10 text-break"><ul> <li style="display:none;">أو بيتا القيطس Beta Ceti اسمه التقليدي Diphda مشتق من الاسم العربي وهو نجم في كوكبة القيطس. ينتمي إلى الفئة الطيفية بين G وK وبالتالي هو نجم مصفر ابرد نوعا ما من الشمس وعلى الرغم من ذلك فهو أكثر ضياء من الشمس وتبلغ كتلته 3 أضعاف كتلة الشمس ونصف قطره حوالي 17 ضعف من نصف قطر الشمس. وهذا النجم انهى مرحلة النسق الأساسي وفي طريقه للتطور إلى مرحلة عملاق أحمر. يبلغ قدره الظاهري 2.04 ويبعد 96 سنة ضوئية عن الأرض اما الضفدع الثاني فيسمى أيضا فم الحوت. (ar)</li> <li style="display:none;">Diphda (Beta de la Balena / β Ceti) és l'estel més brillant de la constel·lació de la Balena. Ocasionalment és superada per la variable Mira (ο Ceti), quan aquesta aconsegueix la seva màxima lluentor. De magnitud aparent de +2,04, és fàcil de localitzar en estar situada en una zona fosca del cel. A la Xina era coneguda com a Too Sze Kung, «el superintendent de les excavacions (edificacions)». (ca)</li> <li style="display:none;">Deneb Kaitos (Beta Ceti, β Cet) je nejjasnější hvězda v souhvězdí Velryby. Přestože je označena „beta“, je ve skutečnosti jasnější než . Jedná se o obra spektrální třídy K0. Lze jej snadno nalézt, neboť v jeho blízkosti nejsou žádné jiné jasné hvězdy. Měřením paralaxy byla zjištěna vzdálenost kolem 96,4 světelných let (29,6 parseků). (cs)</li> <li>Beta Ceti (β Ceti, abbreviated Beta Cet, β Cet), officially named Diphda /ˈdɪfdə/, is the brightest star in the constellation of Cetus. Although designated 'beta', it is actually brighter than the 'alpha' star in the constellation (Alpha Ceti). This orange giant is easy to identify due to its location in an otherwise dark section of the celestial sphere. Based on parallax measurements, it lies at an estimated distance of 96.3 light-years (29.5 parsecs) from the Sun. (en)</li> <li style="display:none;">Deneb Kaitos (β Ceti / 16 Ceti / HD 4128 / HR 188 / HIP 3419) es la estrella más brillante de la constelación de Cetus, la ballena. Ocasionalmente es superada por la variable Mira (ο Ceti), cuando ésta alcanza su máximo brillo.De magnitud aparente de +2,04, es fácil de localizar al estar situada en una zona oscura del cielo. (es)</li> <li style="display:none;">Beta Ceti (β Cet / β Ceti), également appelée par ses noms traditionnels Diphda et Deneb Kaitos, est l'étoile la plus brillante de la constellation de la Baleine. En dépit de sa désignation de Bayer « beta », elle est en réalité plus brillante que Alpha Ceti. Il s'agit d'une étoile géante orangée plus grande et plus lumineuse que le Soleil, qui est de type spectral G9.5 III ou K0 III et qui est donc à la limite entre les étoiles de type G et de type K. (fr)</li> <li style="display:none;">Beta Ceti (β Cet / β Ceti) adalah bintang paling terang di rasi Cetus. Bintang ini mempunyai klasifikasi antara G dan K, membuat bintang ini dirujukkan sebagai bintang yang hampir sama dengan Matahari. Meskipun demikian, bintang ini lebih cemerlang dan lebih besar daripada Matahari. Beta Ceti adalah bintang yang cukup tua dan mendekati tahapan bintang raksasa merah. Dengan magnitudo sebesar 2.04 membuat bintang ini termasuk bintang yang cemerlang di langit malam. Bintang ini berada pada jarak 96 tahun cahaya dari Bumi. (in)</li> <li style="display:none;">くじら座β星は、くじら座の恒星で2等星。 (ja)</li> <li style="display:none;">데네브 카이토스(Deneb Kaitos)는 고래자리에서 가장 밝은 별로, 지구에서 약 96광년 떨어져 있다. 바이어 명명법에 의하면 고래자리 베타이다. 베타임에도 불구하고, 데네브 카이토스는 알파별인 멘카르보다 더 밝다. 고유 명칭은 디프다(Diphda)라고 한다. 데네브 카이토스 주변은 상대적으로 어둡기 때문에 찾기가 쉽다. (ko)</li> <li style="display:none;">Deneb Kaitos (β Cet / β Ceti / Beta Ceti), conosciuta anche come Diphda) è la stella più luminosa della costellazione della Balena, nonostante Bayer le abbia assegnato la lettera β. Il suo nome proprio deriva dall'arabo e significa coda della Balena, mentre il nome alternativo Diphda deriva sempre dall'arabo الضفدع الثاني, al-ḍafdaʿ al-thānī, che significa la seconda rana (essendo invece la prima Fomalhaut). (it)</li> <li style="display:none;">Diphda (Beta Ceti, Deneb Kaitos) – najjaśniejsza gwiazda w gwiazdozbiorze Wieloryba (wielkość gwiazdowa: 2,01m). Odległa od Słońca o około 96 lat świetlnych. (pl)</li> <li style="display:none;">Deneb Kaitos – Diphda, eller Beta Ceti (β Ceti, förkortat Beta Cet, β Cet), som är stjärnans Bayer-beteckning, är en ensam stjärna i sydvästra delen av stjärnbilden Valfisken. Den har en skenbar magnitud av 2,02, är den ljusaste stjärnan i stjärnbilden trots att dess Bayer-beteckning tyder på att den skulle vara näst starkast, och är synlig för blotta ögat. Baserat på parallaxmätningar i Hipparcos-uppdraget på 33,9 mas beräknas den befinna sig på ca 96 ljusårs (30 parsek) avstånd från solen. (sv)</li> <li style="display:none;">Beta Ceti (Deneb Kaitos, Diphda, Difda al Thani, Rana Secunda, 16 Ceti) é uma estrela na direção da Cetus. Possui uma ascensão reta de 00h 43m 35.23s e uma declinação de −17° 59′ 12.1″. Sua magnitude aparente é igual a 2.04. Considerando sua distância de 96 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.30. Pertence à classe espectral K0III. É uma estrela variável suspeita. (pt)</li> <li style="display:none;">土司空（英語：Diphda），也称为鯨魚座β（beta Ceti、简写β Cet）。是鲸鱼座最亮的恒星，视星等为2.02等，绝对星等为−0.31等。土司空位於夜空中的陰暗角落，所以人們可以很容易的觀察到它的位置。因為它距離地球僅96.3光年，所以土司空是距離最近的明亮恆星之一。 (zh)</li> <li style="display:none;">Deneb Kaitos (arab. Schwanz des Ungeheuers) ist die Bezeichnung des Sterns β Ceti (Beta Ceti). Deneb Kaitos hat eine scheinbare Helligkeit von 2,04 mag und ist damit (trotz seiner Bezeichnung) heller als α Ceti und hellster Stern im Sternbild Walfisch. Er ist ein Oranger Riese (Red Clump Star) vom Spektraltyp K0 in einer Entfernung von knapp 100 Lichtjahren (Hipparcos Datenbank).Deneb Kaitos wird manchmal auch Diphda (Frosch) genannt. Andere Namen: Difda al Thani von الضفدع الثاني aḍ-ḍafdaʿ aṯ-ṯānī ‚der zweite Frosch‘ („der erste Frosch“ ist Fomalhaut), sowie gleichbedeutend Rana Secunda. (de)</li> <li style="display:none;">Deneb Kaitos (beta Ceti) is de helderste ster in het sterrenbeeld Walvis (Cetus). De naam is afkomstig uit het Arabisch en staat voor staart van de Walvis. Het Arabische Kaitos is een variant van het Latijnse Cetus.Deneb zonder meer is een andere ster, de staart van de Zwaan. De ster staat ook bekend als Diphda, Difda, Difda al Thani en Rana Secunda. De laatste naam is Spaans en betekent "tweede kikker", de eerste kikker is de ster Fomalhaut in het sterrenbeeld Zuidervis. (nl)</li> <li style="display:none;">Бета Кита — ярчайшая звезда созвездия Кита. Имеет традиционные названия Дифда и Денеб Кайтос. Бета Кита является оранжевым гигантом спектрального класса K0III. Это — старая звезда, которая вступает в финальный этап своего жизненного цикла. Имея массу в 3 массы Солнца, Бета Кита ярче Солнца (болометрически, то есть по всем длинам волн вместе) в 145 раз и в 17 раз больше по диаметру. Температура поверхности звезды составляет около 4500 °C. Расстояние до Земли — 96 световых лет. Видимая звёздная величина +2.04. (ru)</li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://www.w3.org/2000/01/rdf-schema#label">rdfs:label</a> </td><td class="col-10 text-break"><ul> <li style="display:none;">الضفدع الثاني (ar)</li> <li style="display:none;">Diphda (ca)</li> <li style="display:none;">Deneb Kaitos (cs)</li> <li style="display:none;">Deneb Kaitos (de)</li> <li>Beta Ceti (en)</li> <li style="display:none;">Deneb Kaitos (es)</li> <li style="display:none;">Beta Ceti (in)</li> <li style="display:none;">Deneb Kaitos (it)</li> <li style="display:none;">Beta Ceti (fr)</li> <li style="display:none;">데네브 카이토스 (ko)</li> <li style="display:none;">くじら座ベータ星 (ja)</li> <li style="display:none;">Deneb Kaitos (nl)</li> <li style="display:none;">Diphda (pl)</li> <li style="display:none;">Beta Ceti (pt)</li> <li style="display:none;">Бета Кита (ru)</li> <li style="display:none;">Deneb Kaitos (sv)</li> <li style="display:none;">土司空 (zh)</li> </ul></td></tr><tr class="odd"><td class="col-2"><a 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resource="http://ast.dbpedia.org/resource/Deneb_Kaitos" href="http://ast.dbpedia.org/resource/Deneb_Kaitos">http://ast.dbpedia.org/resource/Deneb_Kaitos</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://bs.dbpedia.org/resource/Beta_Ceti" href="http://bs.dbpedia.org/resource/Beta_Ceti">http://bs.dbpedia.org/resource/Beta_Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://ca.dbpedia.org/resource/Diphda" href="http://ca.dbpedia.org/resource/Diphda">dbpedia-ca:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://cs.dbpedia.org/resource/Deneb_Kaitos" href="http://cs.dbpedia.org/resource/Deneb_Kaitos">dbpedia-cs:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://de.dbpedia.org/resource/Deneb_Kaitos" href="http://de.dbpedia.org/resource/Deneb_Kaitos">dbpedia-de:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://es.dbpedia.org/resource/Deneb_Kaitos" href="http://es.dbpedia.org/resource/Deneb_Kaitos">dbpedia-es:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://fa.dbpedia.org/resource/ضفدع_ثانی" href="http://fa.dbpedia.org/resource/ضفدع_ثانی">dbpedia-fa:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://fi.dbpedia.org/resource/Beta_Ceti" href="http://fi.dbpedia.org/resource/Beta_Ceti">dbpedia-fi:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://fr.dbpedia.org/resource/Beta_Ceti" href="http://fr.dbpedia.org/resource/Beta_Ceti">dbpedia-fr:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://he.dbpedia.org/resource/דנב_קאיטוס" href="http://he.dbpedia.org/resource/דנב_קאיטוס">dbpedia-he:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://hi.dbpedia.org/resource/बेटा_सॅटाए_तारा" href="http://hi.dbpedia.org/resource/बेटा_सॅटाए_तारा">http://hi.dbpedia.org/resource/बेटा_सॅटाए_तारा</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://id.dbpedia.org/resource/Beta_Ceti" href="http://id.dbpedia.org/resource/Beta_Ceti">dbpedia-id:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://it.dbpedia.org/resource/Deneb_Kaitos" href="http://it.dbpedia.org/resource/Deneb_Kaitos">dbpedia-it:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://ja.dbpedia.org/resource/くじら座ベータ星" href="http://ja.dbpedia.org/resource/くじら座ベータ星">dbpedia-ja:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://ko.dbpedia.org/resource/데네브_카이토스" href="http://ko.dbpedia.org/resource/데네브_카이토스">dbpedia-ko:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://la.dbpedia.org/resource/Beta_Ceti" href="http://la.dbpedia.org/resource/Beta_Ceti">dbpedia-la:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://lb.dbpedia.org/resource/Deneb_Kaitos_(Stär)" href="http://lb.dbpedia.org/resource/Deneb_Kaitos_(Stär)">dbpedia-lb:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://mk.dbpedia.org/resource/Бета_Кит" href="http://mk.dbpedia.org/resource/Бета_Кит">dbpedia-mk:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://nl.dbpedia.org/resource/Deneb_Kaitos" href="http://nl.dbpedia.org/resource/Deneb_Kaitos">dbpedia-nl:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://pl.dbpedia.org/resource/Diphda" href="http://pl.dbpedia.org/resource/Diphda">dbpedia-pl:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://pt.dbpedia.org/resource/Beta_Ceti" href="http://pt.dbpedia.org/resource/Beta_Ceti">dbpedia-pt:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://ru.dbpedia.org/resource/Бета_Кита" href="http://ru.dbpedia.org/resource/Бета_Кита">dbpedia-ru:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://sk.dbpedia.org/resource/Deneb_Kaitos" href="http://sk.dbpedia.org/resource/Deneb_Kaitos">dbpedia-sk:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://sv.dbpedia.org/resource/Deneb_Kaitos" href="http://sv.dbpedia.org/resource/Deneb_Kaitos">dbpedia-sv:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://sw.dbpedia.org/resource/Chura_(nyota)" href="http://sw.dbpedia.org/resource/Chura_(nyota)">dbpedia-sw:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://tl.dbpedia.org/resource/Beta_Ceti" href="http://tl.dbpedia.org/resource/Beta_Ceti">http://tl.dbpedia.org/resource/Beta_Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://tr.dbpedia.org/resource/Beta_Ceti" href="http://tr.dbpedia.org/resource/Beta_Ceti">dbpedia-tr:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://vi.dbpedia.org/resource/Beta_Ceti" href="http://vi.dbpedia.org/resource/Beta_Ceti">dbpedia-vi:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="http://zh.dbpedia.org/resource/土司空" href="http://zh.dbpedia.org/resource/土司空">dbpedia-zh:Beta Ceti</a></li> <li><a class="uri" rel="owl:sameAs" resource="https://global.dbpedia.org/id/LSJu" href="https://global.dbpedia.org/id/LSJu">https://global.dbpedia.org/id/LSJu</a></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://www.w3.org/ns/prov#wasDerivedFrom">prov:wasDerivedFrom</a> </td><td class="col-10 text-break"><ul> <li><a class="uri" rel="prov:wasDerivedFrom" resource="http://en.wikipedia.org/wiki/Beta_Ceti?oldid=1115176056&ns=0" href="http://en.wikipedia.org/wiki/Beta_Ceti?oldid=1115176056&ns=0">wikipedia-en:Beta_Ceti?oldid=1115176056&ns=0</a></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://xmlns.com/foaf/0.1/depiction">foaf:depiction</a> </td><td class="col-10 text-break"><ul> <li><a class="uri" rel="foaf:depiction" resource="http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg" href="http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg">wiki-commons:Special:FilePath/Red_circle.svg</a></li> <li><a class="uri" rel="foaf:depiction" resource="http://commons.wikimedia.org/wiki/Special:FilePath/Cetus_constellation_map.svg" href="http://commons.wikimedia.org/wiki/Special:FilePath/Cetus_constellation_map.svg">wiki-commons:Special:FilePath/Cetus_constellation_map.svg</a></li> <li><a class="uri" rel="foaf:depiction" resource="http://commons.wikimedia.org/wiki/Special:FilePath/Bceti_xray.jpg" href="http://commons.wikimedia.org/wiki/Special:FilePath/Bceti_xray.jpg">wiki-commons:Special:FilePath/Bceti_xray.jpg</a></li> <li><a class="uri" rel="foaf:depiction" resource="http://commons.wikimedia.org/wiki/Special:FilePath/BetaCetLightCurve.png" href="http://commons.wikimedia.org/wiki/Special:FilePath/BetaCetLightCurve.png">wiki-commons:Special:FilePath/BetaCetLightCurve.png</a></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://xmlns.com/foaf/0.1/isPrimaryTopicOf">foaf:isPrimaryTopicOf</a> </td><td class="col-10 text-break"><ul> <li><a class="uri" rel="foaf:isPrimaryTopicOf" resource="http://en.wikipedia.org/wiki/Beta_Ceti" href="http://en.wikipedia.org/wiki/Beta_Ceti">wikipedia-en:Beta_Ceti</a></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://xmlns.com/foaf/0.1/name">foaf:name</a> </td><td class="col-10 text-break"><ul> <li>β Ceti (en)</li> </ul></td></tr><tr class="even"><td class="col-2">is <a class="uri" href="http://dbpedia.org/ontology/wikiPageRedirects">dbo:wikiPageRedirects</a> of</td><td class="col-10 text-break"><ul> <li><a class="uri" rev="dbo:wikiPageRedirects" resource="http://dbpedia.org/resource/Beta_Cet" href="http://dbpedia.org/resource/Beta_Cet">dbr:Beta_Cet</a></li> <li><a class="uri" rev="dbo:wikiPageRedirects" resource="http://dbpedia.org/resource/HIP_3419" href="http://dbpedia.org/resource/HIP_3419">dbr:HIP_3419</a></li> <li><a class="uri" rev="dbo:wikiPageRedirects" resource="http://dbpedia.org/resource/Β_Cet" href="http://dbpedia.org/resource/Β_Cet">dbr:Β_Cet</a></li> <li><a class="uri" rev="dbo:wikiPageRedirects" resource="http://dbpedia.org/resource/Β_Ceti" href="http://dbpedia.org/resource/Β_Ceti">dbr:Β_Ceti</a></li> <li><a class="uri" rev="dbo:wikiPageRedirects" resource="http://dbpedia.org/resource/Diphda" href="http://dbpedia.org/resource/Diphda">dbr:Diphda</a></li> <li><a class="uri" rev="dbo:wikiPageRedirects" resource="http://dbpedia.org/resource/Diphda_(star)" href="http://dbpedia.org/resource/Diphda_(star)">dbr:Diphda_(star)</a></li> <li><a class="uri" rev="dbo:wikiPageRedirects" resource="http://dbpedia.org/resource/16_Cet" href="http://dbpedia.org/resource/16_Cet">dbr:16_Cet</a></li> <li><a class="uri" rev="dbo:wikiPageRedirects" resource="http://dbpedia.org/resource/16_Ceti" href="http://dbpedia.org/resource/16_Ceti">dbr:16_Ceti</a></li> <li><a class="uri" rev="dbo:wikiPageRedirects" resource="http://dbpedia.org/resource/Difda" href="http://dbpedia.org/resource/Difda">dbr:Difda</a></li> </ul></td></tr><tr class="odd"><td class="col-2">is <a class="uri" href="http://dbpedia.org/ontology/wikiPageWikiLink">dbo:wikiPageWikiLink</a> of</td><td class="col-10 text-break"><ul> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Beta_Cet" href="http://dbpedia.org/resource/Beta_Cet">dbr:Beta_Cet</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Deneb" href="http://dbpedia.org/resource/Deneb">dbr:Deneb</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/USS_Diphda_(AKA-59)" href="http://dbpedia.org/resource/USS_Diphda_(AKA-59)">dbr:USS_Diphda_(AKA-59)</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/12P/Pons–Brooks" href="http://dbpedia.org/resource/12P/Pons–Brooks">dbr:12P/Pons–Brooks</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Chinese_star_names" href="http://dbpedia.org/resource/Chinese_star_names">dbr:Chinese_star_names</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Cetus" href="http://dbpedia.org/resource/Cetus">dbr:Cetus</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/List_of_Arabic_star_names" href="http://dbpedia.org/resource/List_of_Arabic_star_names">dbr:List_of_Arabic_star_names</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Red_clump" href="http://dbpedia.org/resource/Red_clump">dbr:Red_clump</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Table_of_stars_with_Bayer_designations" href="http://dbpedia.org/resource/Table_of_stars_with_Bayer_designations">dbr:Table_of_stars_with_Bayer_designations</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Alpha_Ceti" href="http://dbpedia.org/resource/Alpha_Ceti">dbr:Alpha_Ceti</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Fomalhaut" href="http://dbpedia.org/resource/Fomalhaut">dbr:Fomalhaut</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Deneb_Kaitos" href="http://dbpedia.org/resource/Deneb_Kaitos">dbr:Deneb_Kaitos</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Legs_(Chinese_constellation)" href="http://dbpedia.org/resource/Legs_(Chinese_constellation)">dbr:Legs_(Chinese_constellation)</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Phoenix_(constellation)" href="http://dbpedia.org/resource/Phoenix_(constellation)">dbr:Phoenix_(constellation)</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/HIP_3419" href="http://dbpedia.org/resource/HIP_3419">dbr:HIP_3419</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Cetus_in_Chinese_astronomy" href="http://dbpedia.org/resource/Cetus_in_Chinese_astronomy">dbr:Cetus_in_Chinese_astronomy</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Sculptor_Galaxy" href="http://dbpedia.org/resource/Sculptor_Galaxy">dbr:Sculptor_Galaxy</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Table_of_stars_with_Flamsteed_designations" href="http://dbpedia.org/resource/Table_of_stars_with_Flamsteed_designations">dbr:Table_of_stars_with_Flamsteed_designations</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/IAU_designated_constellations" href="http://dbpedia.org/resource/IAU_designated_constellations">dbr:IAU_designated_constellations</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/List_of_stars_for_navigation" href="http://dbpedia.org/resource/List_of_stars_for_navigation">dbr:List_of_stars_for_navigation</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/List_of_stars_in_Cetus" href="http://dbpedia.org/resource/List_of_stars_in_Cetus">dbr:List_of_stars_in_Cetus</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Β_Cet" href="http://dbpedia.org/resource/Β_Cet">dbr:Β_Cet</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Β_Ceti" href="http://dbpedia.org/resource/Β_Ceti">dbr:Β_Ceti</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/List_of_brightest_natural_objects_in_the_sky" href="http://dbpedia.org/resource/List_of_brightest_natural_objects_in_the_sky">dbr:List_of_brightest_natural_objects_in_the_sky</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Diphda" href="http://dbpedia.org/resource/Diphda">dbr:Diphda</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Diphda_(star)" href="http://dbpedia.org/resource/Diphda_(star)">dbr:Diphda_(star)</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/16_Cet" href="http://dbpedia.org/resource/16_Cet">dbr:16_Cet</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/16_Ceti" href="http://dbpedia.org/resource/16_Ceti">dbr:16_Ceti</a></li> <li><a class="uri" rev="dbo:wikiPageWikiLink" resource="http://dbpedia.org/resource/Difda" href="http://dbpedia.org/resource/Difda">dbr:Difda</a></li> </ul></td></tr><tr class="even"><td class="col-2">is <a class="uri" href="http://xmlns.com/foaf/0.1/primaryTopic">foaf:primaryTopic</a> of</td><td class="col-10 text-break"><ul> <li><a class="uri" rev="foaf:primaryTopic" resource="http://en.wikipedia.org/wiki/Beta_Ceti" href="http://en.wikipedia.org/wiki/Beta_Ceti">wikipedia-en:Beta_Ceti</a></li> </ul></td></tr> </tbody> </table> </div> </div> </div> </section>   <section> <div class="container-xl"> <div class="text-center p-4 bg-light"> <a href="https://virtuoso.openlinksw.com/" title="OpenLink Virtuoso"><img class="powered_by" src="/statics/images/virt_power_no_border.png" alt="Powered by OpenLink Virtuoso"/></a>    <a href="http://linkeddata.org/"><img alt="This material is Open Knowledge" src="/statics/images/LoDLogo.gif"/></a>     <a href="http://dbpedia.org/sparql"><img alt="W3C Semantic Web Technology" src="/statics/images/sw-sparql-blue.png"/></a>     <a href="https://opendefinition.org/"><img alt="This material is Open Knowledge" src="/statics/images/od_80x15_red_green.png"/></a>    <a href="https://validator.w3.org/check?uri=referer"> <img src="https://www.w3.org/Icons/valid-xhtml-rdfa" alt="Valid XHTML + RDFa" /> </a> This content was extracted from <a 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