Dzeimsa Veba teleskopa pirmie atteli sajusmina pasauli

Published: July 26, 2022, 8:07 a.m.

b'Pirmie Veba teleskopa att\\u0113li saj\\u016bsmin\\u0101ju\\u0161i ne tikai astronomus, bet cilv\\u0113kus vis\\u0101 pasaul\\u0113. D\\u017eeimsa Veba teleskops ir pav\\u0113ris mums lappuses vissen\\u0101kaj\\u0101 v\\u0113stures gr\\u0101mat\\u0101 par Visumu. Taj\\u0101 redzam galaktikas no pa\\u0161iem Visuma pirms\\u0101kumiem. Kr\\u0101\\u0161\\u0146ajos att\\u0113los skat\\u0101mas pat 13 miljardus gadu senas galaktikas un dramatiskas migl\\u0101ju ainavas.\\n\\nKo \\u0161ie att\\u0113li mums pal\\u012bdz\\u0113s uzzin\\u0101t par Visuma v\\u0113sturi, raid\\u012bjum\\u0101 Zin\\u0101mais nezin\\u0101maj\\u0101 st\\u0101sta amatierastronomi un interneta tehnolo\\u0123iju speci\\u0101listi Raitis Misa un Ints \\u0136e\\u0161\\u0101ns.\\n\\nZin\\u0101mais nezin\\u0101maj\\u0101 ar\\u012b st\\u0101sts par zvaig\\u017e\\u0146u dzim\\u0161anu. Proti, veroties debes\\u012bs, zvaigznes m\\u0113s redzam k\\u0101 spo\\u017eus punktus. Diezin vai \\u0161aj\\u0101 br\\u012bd\\u012b tik daudz aizdom\\u0101jamies par to, ka zvaig\\u017e\\u0146u dz\\u012bv\\u0113 nov\\u0113rojamas ar\\u012b t\\u0101das stadijas k\\u0101 baltais punduris, br\\u016bnais punduris un v\\u0113l citas. Bet skaidrs ir tas, ka zvaigznes no kaut k\\u0101 rodas, t\\u0101s savas dz\\u012bves laik\\u0101 main\\u0101s un kaut kad to dz\\u012bve ar\\u012b izbeidzas. Par zvaig\\u017e\\u0146u da\\u017e\\u0101diem dz\\u012bves posmiem vair\\u0101k st\\u0101sta Latvijas Astronomijas biedr\\u012bbas projektu vad\\u012bt\\u0101js M\\u0101rti\\u0146\\u0161 Gills.\\n\\nT\\u0101tad zvaigznes piedzimst, s\\u0101kum\\u0101 no t\\u012bra \\u016bde\\u0146ra\\u017ea, bet v\\u0113l\\u0101k no da\\u017e\\u0101du atomu, element\\u0101rda\\u013ci\\u0146u un zvaig\\u017e\\u0146u putek\\u013cu bu\\u0137etes. Var b\\u016bt pavisam vieglas zvaigzn\\u012btes, kuras pa \\u012bstam neuzliesmo un t\\u0101 ar\\u012b izdziest. Un var b\\u016bt ar\\u012b spo\\u017eas zvaigznes ar lielu masu, kuru dz\\u012bves turpin\\u0101jums raksturojams ar da\\u017e\\u0101d\\u0101m izpausm\\u0113m, proti, Supernovas spr\\u0101dzieni, Melnie caurumi, magnet\\u0101ras, k\\u0101 ar\\u012b Sarkanie mil\\u017ei, da\\u017e\\u0101du kr\\u0101su punduri un ne tik tas vien.'