. . .
BPM 37093은 지구로부터 센타우루스자리 방향으로
53광년 떨어져 있는 분광형 백색 왜성입니다.
이 항성의크기는 매우 작은 경우인데
반지름이 수성보다도 작습니다
표면온도는 11,730K이고.
. . .
페르미 액체에 둘러싸인, 탄소 등으로 인한
산소 원자핵 입방정계 구조로 되어 있어서
과학자들은 이 항성의 내부 중심부에
다이아몬드와 유사한 물질로 가득 채워져 있을 것으로
추정합니다.
Source : https://www.youtube.com/channel/UCmHof0uMcf-KZOZfxmbRrOw/about?view_as=subscriber
Image Source :
https://commons.wikimedia.org/wiki/File:Alpha,_Beta_and_Proxima_Centauri_(1).jpg
https://commons.wikimedia.org/wiki/File:Relative_positions_of_Sun,_Alpha_Centauri_AB_and_Proxima_Centauri.png
https://commons.wikimedia.org/wiki/File:Alpha_Centauri_relative_sizes.svg
https://commons.wikimedia.org/wiki/File:Best_image_of_Alpha_Centauri_A_and_B.jpg
https://commons.wikimedia.org/wiki/File:Orbit_Alpha_Centauri_AB_arcsec.png
https://commons.wikimedia.org/wiki/File:Artist%E2%80%99s_impression_of_Proxima_Centauri_b_shown_hypothetically_as_an_arid_rocky_super-earth.jpg
https://commons.wikimedia.org/wiki/File:Artist%27s_impression_of_the_planet_orbiting_Proxima_Centauri.jpg
https://commons.wikimedia.org/wiki/File:Artist%E2%80%99s_impression_of_a_planet_around_Alpha_Centauri_B_(symbolic,_annotated).jpg
https://commons.wikimedia.org/wiki/File:Virgo_constellation_map.svg
https://commons.wikimedia.org/wiki/File:Regulus_1.JPG
https://commons.wikimedia.org/wiki/File:Sigma_Draconis.jpg
https://commons.wikimedia.org/wiki/File:Iades_and_Pleiades_(32446251210).jpg
https://commons.wikimedia.org/wiki/File:Leo_constellation_map.png
https://commons.wikimedia.org/wiki/File:Gemini_IAU.svg
https://commons.wikimedia.org/wiki/File:P%C3%B3lux_B.jpg
https://commons.wikimedia.org/wiki/File:Kapteyn%27s_Star_Comparison.jpg
https://commons.wikimedia.org/wiki/File:Orbit_Sirius_B_arcsec.png
https://commons.wikimedia.org/wiki/File:WR-134.png
https://commons.wikimedia.org/wiki/File:Sadr_Region_rgb.jpg
https://en.wikipedia.org/wiki/File:Carina_Nebula_by_ESO.jpg
https://commons.wikimedia.org/wiki/File:The_brilliant_star_VFTS_682_in_the_Large_Magellanic_Cloud.jpg
https://commons.wikimedia.org/wiki/File:Stephenson_2-18_zoomed_in,_2MASS_survey,_2003.png
https://commons.wikimedia.org/wiki/File:1806-20_cluster.jpg
https://commons.wikimedia.org/wiki/File:ESO_-_Eso1030a_(by).jpg
https://commons.wikimedia.org/wiki/File:The_young_cluster_R136.jpg
https://commons.wikimedia.org/wiki/File:Stephenson_2_DFK_1_seen_by_PanSTARRS_DR1.png
https://commons.wikimedia.org/wiki/File:Brown_Dwarf_Binary_CFBDSIR_1458%2B10.tif
https://commons.wikimedia.org/wiki/File:Oldest_star_in_solar_neighbourhood.jpg
https://commons.wikimedia.org/wiki/File:Stephenson2-18.svg
https://www.yna.co.kr/view/AKR20220823035100009?section=search
https://commons.wikimedia.org/wiki/File:Webb%E2%80%99s_Jupiter_Images_Showcase_Auroras,_Hazes_-_52303461859.png
https://commons.wikimedia.org/wiki/File:Webb%E2%80%99s_Jupiter_Images_Showcase_Auroras,_Hazes_-_52302207952.png
https://commons.wikimedia.org/wiki/File:New_shot_of_Proxima_Centauri,_our_nearest_neighbour.jpg
https://commons.wikimedia.org/wiki/File:Alpha_centauri_size.png
https://commons.wikimedia.org/wiki/File:Lalande_21185.png
https://commons.wikimedia.org/wiki/File:Ross_248_1.D4.jpg
https://commons.wikimedia.org/wiki/File:Artist%27s_impression_of_the_planet_Ross_128_b.jpg
https://commons.wikimedia.org/wiki/File:Compare_sun_tau_ceti.png
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