A type stars are bigger and hotter than our Sun, A type main-sequence star mass is around 1.4 to 2.1 solar masses and size 1.6 to 2.4 solar radii.
In this 3d visualization we will see the size of A type main sequence and giant stars compared to our Sun which is a G-type main-sequence star 4.6 billion years old.
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#starsizecomparison #Atypestars #blender
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https://www.youtube.com/watch?v=DizhZS9XPsI
CEERS-93316 candidate farthest galaxy ever found 13.7 billion light-years away, 34.9 billion light-years (current proper distance). Existed just 236 million years after Big Bang. The Red Shift of 16.4
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https://www.youtube.com/watch?v=WtNhFBXLW0o
Segue 2 is a dwarf spheroidal galaxy situated in the constellation Aries and discovered in 2009 in the data obtained by Sloan Digital Sky Survey. The galaxy is located at the distance of about 35 kiloparsecs (35,000 parsecs; 110,000 light-years) from the Sun
सेग 2 एक बौनी गोलाकार आकाशगंगा है जो मेष राशि में स्थित है और 2009 में स्लोन डिजिटल स्काई सर्वे द्वारा प्राप्त आंकड़ों में खोजी गई थी। आकाशगंगा सूर्य से लगभग 35 किलोपारसेक (35,000 पारसेक; 110,000 प्रकाश वर्ष) की दूरी पर स्थित है
Segue 2 — карликовая сфероидальная галактика, расположенная в созвездии Овна и обнаруженная в 2009 году в данных, полученных Sloan Digital Sky Survey. Галактика расположена на расстоянии около 35 килопарсеков (35 000 парсеков; 110 000 световых лет) от Солнца.
Segue 2 é uma galáxia anã esferoidal situada na constelação de Áries e descoberta em 2009 nos dados obtidos pelo Sloan Digital Sky Survey. A galáxia está localizada a uma distância de cerca de 35 kiloparsecs (35.000 parsecs; 110.000 anos-luz) do Sol
Ang Segue 2 ay isang dwarf spheroidal galaxy na matatagpuan sa konstelasyon ng Aries at natuklasan noong 2009 sa data na nakuha ng Sloan Digital Sky Survey. Ang kalawakan ay matatagpuan sa layo na humigit-kumulang 35 kiloparsec (35,000 parsec; 110,000 light-years) mula sa Araw
Segue 2 adalah galaksi bola kerdil yang terletak di konstelasi Aries dan ditemukan pada tahun 2009 dalam data yang diperoleh Sloan Digital Sky Survey. Galaksi terletak pada jarak sekitar 35 kiloparsec (35.000 parsec; 110.000 tahun cahaya) dari Matahari
Music from pixabay.com
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#astronomy #science #spaceengine
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https://www.youtube.com/watch?v=AVFrQG1OURE
KELT-11b puffy planet in space engine
KELT-11 is a subgiant star host a puffy planet KELT-11b, planet's mass is 20% of Jupiter and size is 14.5 times of Earth, almost 50% bigger than Jupiter.
In this video we will explore the KELT-11b puffy planet in space engine universe simulator.
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#KELT11b #exoplanet #spaceengine
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https://www.youtube.com/watch?v=S73t--iihWk
Kepler-90d Space Engine
In this video we will explore the exoplanet Kepler-90d in space engine universe simulator.
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#Kepler90d #exoplanet #spaceengine
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https://www.youtube.com/watch?v=4Rv-kQoCXkQ
This is NGC 6752, Great Peacock Globular 13000 light-years away from solar system, fourth brightest globular cluster in the sky. in Space Engine.
What is a Globular Cluster ?
A globular cluster is a spheroidal shape of group of stars. Globular clusters are bound together by gravity, with a higher concentration of stars towards their centers.
In spiral galaxies like the Milky Way they are mostly found in the outer spheroidal part of the galaxy, the galactic halo.
Milky Way has more than 150 known globular clusters, and there may be many more.
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#astronomy #science #spaceengine #gameplay #exoplanet #space #exploremore #real
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https://www.youtube.com/watch?v=RyJXt-hkA50
K type Stars Orange dwarf , Orange giant stars Size Comparison,
'V' denotes its luminosity class main sequence , 'III' denotes luminosity class of giant evolved stars whose surface temperature ranges from 5000 to 3700 kelvin. K type main-sequence star is smaller than Sun which is a G type star, and has cooler temperature than sun which gives them orange hue.
In this video we will see the size of K-type dwarf star and giant stars as compare to our sun which is a G-type main-sequence star 4.6 billion years old.
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K प्रकार के सितारे नारंगी बौना, नारंगी विशाल सितारे आकार तुलना,
'वी' अपने चमकदार वर्ग मुख्य अनुक्रम को दर्शाता है, 'III' विशाल विकसित सितारों के चमकदार वर्ग को दर्शाता है जिनकी सतह का तापमान 5000 से 3700 केल्विन तक होता है। K प्रकार का मुख्य अनुक्रम तारा सूर्य से छोटा होता है जो कि G प्रकार का तारा है, और इसका तापमान सूर्य की तुलना में ठंडा होता है जो उन्हें नारंगी रंग देता है।
इस वीडियो में हम अपने सूर्य की तुलना में K-प्रकार के बौने तारे और विशाल सितारों के आकार को देखेंगे जो कि 4.6 बिलियन वर्ष पुराना G-प्रकार का मुख्य-अनुक्रम तारा है।
#KtypeStar #OrangeDwarf #blender
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https://www.youtube.com/watch?v=oTDSO8XGbLY