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Kelaikhunian satelit alami 위성 거주가능성 Abitabilità di un satellite naturale قابلية الأقمار الطبيعية للحياة Habitabilidade de satélites naturais Habitability of natural satellites
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The habitability of natural satellites is a measure of their potential to sustain life in favorable circumstances. Habitable environments do not necessarily harbor life. Natural satellite habitability is a new area that is significant to astrobiology for various reasons, the most important of which being that natural satellites are expected to outnumber planets by a large margin, and it is projected that habitability parameters will be comparable to those of planets. There are, nevertheless, significant environmental variables that affect moons as prospective alien life locations.The strongest candidates for natural satellite habitability are currently icy satellites such as those of Jupiter and Saturn—Europa and Enceladus respectively, although if life exists in either place, it would pro L'abitabilità dei satelliti naturali si riferisce alla capacità potenziale dei satelliti naturali di avere ambienti ospitali alla vita, anche se gli ambienti abitabili non ospitano necessariamente la vita. L'abitabilità satellitare è uno studio emergente considerato importante per l'astrobiologia per diversi motivi, soprattutto perché si suppone che i satelliti naturali siano notevolmente più numerosi dei pianeti e si ipotizza che i fattori di abitabilità siano probabilmente simili a quelli dei pianeti. 위성 거주가능성은 자연 위성에 생명체가 자라나고 유지될 수 있는 가능성을 측정하는 것이다. 현재 태양계에는 생명이 있는 것으로 알려진 위성이 없다. 태양계의 생명체 거주가능 영역에는 달, 포보스, 데이모스가 있지만 이들 천체에는 액체나 대기가 없어 생명이 없을 것으로 생각된다. 몇몇 과학자들은 목성, 토성의 위성에 생명이 있을 것으로 생각한다. 현재 외계 위성은 하나도 발견되지 않은 상태이다. Kelaikhunian satelit alami adalah sebuah ukuran potensi satelit alami untuk memiliki lingkungan yang ramah untuk kehidupan. Lingkungan yang laik huni tidak selalu mengandung kehidupan. قابلية الأقمار الطبيعية للحياة هو مقياس لقدرة الأقمار الطبيعية لتكون بيئات مضيافة للحياة. البيئات القابلة للسكنى لا تؤمن بالضرورة الحياة. وتعتبر قابلية الكواكب دراسة ناشئة تعتبر هامة لعلم الأحياء الفلكية لعدة أسباب، أهمها أن الأقمار الطبيعية يتوقع أن تفوق عدد الكواكب إلى حد كبير ومن المفترض أن تكون عوامل قابلية السكن في الأقمار الطبيعية مشابهة لتلك الموجودة في الكواكب. وأقوى مرشحي الأقمار الطبيعية لاستضافة الحياة حاليا هي الأقمار الجليدية على سبيل المثال قمر المشتري أوروبا وقمر زحل إنسيلادوس على الرغم من أنه إذا كانت الحياة موجودة في أي من هما، فمن المحتمل أن تكون تحت السطح.وتاريخيا، كان يعتقد أن الحياة على الأرض هي ظاهرة سطحية تماما، ولكن الدراسات الحديثة أظهرت أن ما يصل إلى نصف الكتلة الحيوية للأرض يمكن أن تعيش تحت سطح الأرض.
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Kelaikhunian satelit alami adalah sebuah ukuran potensi satelit alami untuk memiliki lingkungan yang ramah untuk kehidupan. Lingkungan yang laik huni tidak selalu mengandung kehidupan. L'abitabilità dei satelliti naturali si riferisce alla capacità potenziale dei satelliti naturali di avere ambienti ospitali alla vita, anche se gli ambienti abitabili non ospitano necessariamente la vita. L'abitabilità satellitare è uno studio emergente considerato importante per l'astrobiologia per diversi motivi, soprattutto perché si suppone che i satelliti naturali siano notevolmente più numerosi dei pianeti e si ipotizza che i fattori di abitabilità siano probabilmente simili a quelli dei pianeti. Vi sono, tuttavia, differenze chiave che incidono sulle lune come potenziali siti per la vita extraterrestre. I candidati più probabili all'abitabilità dei satelliti naturali sono attualmente i satelliti ghiacciati come quelli di Giove e Saturno - Europa ed Encelado rispettivamente, sebbene anche se la vita esistesse in entrambi i luoghi, sarebbe probabilmente limitata agli habitat al di sotto della crosta superficiale. Tradizionalmente, si riteneva che la vita sulla Terra fosse strettamente un fenomeno di superficie, ma recenti studi hanno dimostrato che fino alla metà della biomassa terrestre potrebbe vivere al di sotto della superficie. Europa ed Encelado esistono al di fuori della zona abitabile circumstellare che ha per lungo tempo definito i limiti della vita all'interno del sistema solare come la zona in cui l'acqua può esistere allo stato liquido in superficie. Nella zona abitabile del sistema solare ci sono solo tre satelliti naturali: la Luna e le lune di Marte Phobos e Deimos (anche se alcune stime evidenziano che Marte e le sue lune sono leggermente al di fuori della zona abitabile) nessuno dei quali sostiene un'atmosfera o acqua in forma liquida. È probabile che le forze di marea svolgano un ruolo altrettanto significativo fornendo calore al pari delle radiazioni stellari nella potenziale abitabilità dei satelliti naturali. Non è ancora stata confermata l'esistenza di esolune. Rilevarle è estremamente difficile, perché gli attuali metodi sono limitati ai tempi di transito. È possibile che alcune delle loro proprietà possano essere determinate con metodi simili a quelli dei pianeti in transito. Nonostante ciò, alcuni scienziati stimano che ci siano tante esolune abitabili quanti esopianeti abitabili. Dato il rapporto generale di massa da pianeta a satellite/i di 10 000:1, grandi pianeti gassosi delle dimensioni di Saturno o Giove nella zona abitabile sono considerati i migliori candidati per ospitare lune simili alla Terra. 위성 거주가능성은 자연 위성에 생명체가 자라나고 유지될 수 있는 가능성을 측정하는 것이다. 현재 태양계에는 생명이 있는 것으로 알려진 위성이 없다. 태양계의 생명체 거주가능 영역에는 달, 포보스, 데이모스가 있지만 이들 천체에는 액체나 대기가 없어 생명이 없을 것으로 생각된다. 몇몇 과학자들은 목성, 토성의 위성에 생명이 있을 것으로 생각한다. 현재 외계 위성은 하나도 발견되지 않은 상태이다. قابلية الأقمار الطبيعية للحياة هو مقياس لقدرة الأقمار الطبيعية لتكون بيئات مضيافة للحياة. البيئات القابلة للسكنى لا تؤمن بالضرورة الحياة. وتعتبر قابلية الكواكب دراسة ناشئة تعتبر هامة لعلم الأحياء الفلكية لعدة أسباب، أهمها أن الأقمار الطبيعية يتوقع أن تفوق عدد الكواكب إلى حد كبير ومن المفترض أن تكون عوامل قابلية السكن في الأقمار الطبيعية مشابهة لتلك الموجودة في الكواكب. وأقوى مرشحي الأقمار الطبيعية لاستضافة الحياة حاليا هي الأقمار الجليدية على سبيل المثال قمر المشتري أوروبا وقمر زحل إنسيلادوس على الرغم من أنه إذا كانت الحياة موجودة في أي من هما، فمن المحتمل أن تكون تحت السطح.وتاريخيا، كان يعتقد أن الحياة على الأرض هي ظاهرة سطحية تماما، ولكن الدراسات الحديثة أظهرت أن ما يصل إلى نصف الكتلة الحيوية للأرض يمكن أن تعيش تحت سطح الأرض. الأقمار خارج المجموعة الشمسية لم يتم التأكد بعد من وجودها ورصدها أمر صعب للغاية، لأن الطرق الحالية تقتصر على توقيت العبور . ومن الممكن أن بعض سماتها يمكن تحديدها بطرق مماثلة لطرق عبور الكواكب (transiting planets.). وعلى الرغم من هذ افأن بعض العلماء يقدرون أن هناك العديد من الأقمار خارج المجموعة الشمسية صالحة للسكن كعدد الكواكب خارج المجموعة الشمسية الصالحة للسكن The habitability of natural satellites is a measure of their potential to sustain life in favorable circumstances. Habitable environments do not necessarily harbor life. Natural satellite habitability is a new area that is significant to astrobiology for various reasons, the most important of which being that natural satellites are expected to outnumber planets by a large margin, and it is projected that habitability parameters will be comparable to those of planets. There are, nevertheless, significant environmental variables that affect moons as prospective alien life locations.The strongest candidates for natural satellite habitability are currently icy satellites such as those of Jupiter and Saturn—Europa and Enceladus respectively, although if life exists in either place, it would probably be confined to subsurface habitats. Historically, life on Earth was thought to be strictly a surface phenomenon, but recent studies have shown that up to half of Earth's biomass could live below the surface. Europa and Enceladus exist outside the circumstellar habitable zone which has historically defined the limits of life within the Solar System as the zone in which water can exist as liquid at the surface. In the Solar System's habitable zone, there are only three natural satellites—the Moon, and Mars's moons Phobos and Deimos (although some estimates show Mars and its moons to be slightly outside the habitable zone) —none of which sustain an atmosphere or water in liquid form. Tidal forces are likely to play as significant a role providing heat as stellar radiation in the potential habitability of natural satellites. Exomoons are not yet confirmed to exist. Detecting them is extremely difficult, because current methods are limited to transit timing. It is possible that some of their attributes could be determined by similar methods as those of transiting planets. Despite this, some scientists estimate that there are as many habitable exomoons as habitable exoplanets. Given the general planet-to-satellite(s) mass ratio of 10,000, large Saturn or Jupiter sized gas planets in the habitable zone are thought to be the best candidates to harbour Earth-like moons.
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