Áú¹®/´äº¯
ºê·£µåÀåÁ¡
ÀÎÁõ¼­
ÇÁ·Î±×·¥ º¸±â
¼ö°­½Åû/ºñ¿ëº¸±â
ƼÃĵ¿¿µ»ó
¿¬¼ö¼ö±â
Æ÷Åä°¶·¯¸®
¸ÞÀιè³Ê
  • Çпø¼Ò°³
  • À×±Û¸®½¬700ÇÁ·Î±×·¥
  • ¼ö°­½Åû/ºñ¿ë
  • ·¹º§Å×½ºÆ®
  • À¯Çп¬¼öÇÁ·Î±×·¥
  • À¯Çп¬¼öÁغñ/½Åû
  • Ä¿¹Â´ÏƼ
  • Ȩ > Ä¿¹Â´ÏƼ > Today's Issue
    °øÁö»çÇ×
    Áú¹® ¹× ´äº¯
    ¿¬¼öÈıâ/ÁøÇÐÈıâ
    Æ÷Åä°¶·¯¸®
    ¾îÇпø¸ð½À
    ¼ö¾÷µ¿¿µ»ó ¼±»ý´Ô¼Ò°³
    ºê·»Æ®±¹Á¦Çб³ ½Ç½Ã°£Á¤º¸
    ºñ±â³Ê¸¦ À§ÇÑ º¸Ä«ÀÇÀÌÇØ
    ¿øÀåÀÇ ÃÌö»ìÀÎ Ä®·³
    ÀαâÄÁÅÙÃ÷ TOP 10
    Today's Issue
    µ¿¿µ»ó ¼Ó ¿µ¾î
    ¼±»ý´Ôµ¿¿µ»ó°­ÀÇ
    Ä¿¹Â´ÏƼ
    °øÁö»çÇ×
    Áú¹®¹×´äº¯
    ¿¬¼öÈıâ/ÁøÇÐÈıâ
    Æ÷Åä°¶·¯¸®
    ¾îÇпø¸ð½À
    ¼ö¾÷µ¿¿µ»ó ¼±»ý´Ô¼Ò°³
    Á¹¾÷»ýµéÀÇ Á¶¾ð
    ºñ±â³Ê¸¦ À§ÇÑ º¸Ä«ÀÇÀÌÇØ
    ¿øÀåÀÇ ÃÌö»ìÀÎ Ä®·³
    ÀαâÄÁÅÙÃ÷ TOP 10
    ÷»è°Ô½ÃÆÇ
    ¼ö¾÷´ëº»°Ô½ÃÆÇ
    ¼±»ý´Ôµ¿¿µ»ó°­ÀÇ
     
    Today's Issue
    ¿µ¾î±³À°ÀÇ Á¤Á¡ À×±Û¸®½¬ 700ÀÔ´Ï´Ù.
    Today's Issue
    ¿µ¾î±³À°ÀÇ Á¤Á¡ À×±Û¸®½¬ 700ÀÔ´Ï´Ù.
     
    Çظ¦ Ç°Àº ´Þ °³±âÀϽÄ
    ÀÌ    ¸§     |     °ü¸®ÀÚ µî·ÏÀÏ     |     2024-04-09 Á¶    È¸     |     837
    ÀÌ    ¸§     |     °ü¸®ÀÚ Á¶    È¸     |     837
    µî·ÏÀÏ     |     2024-04-09

    Total solar eclipse

     

     

     

    The moon fully blocked the sun in parts of Canada, Mexico and the US, drawing the attention of star-gazers and scientists.

    ´ÞÀº ij³ª´Ù, ¸ß½ÃÄÚ, ¹Ì±¹ ÀϺΠÁö¿ª¿¡¼­ žçÀ» ¿ÏÀüÈ÷ °¡·Á º°À» °üÃøÇÏ´Â »ç¶÷µé°ú °úÇÐÀÚµéÀÇ °ü½ÉÀ» ²ø¾ú½À´Ï´Ù.

     

     

    On Monday, parts of Canada, Mexico and the United States were treated to a total solar eclipse, a phenomenon that will not arise for another two decades.

    ¿ù¿äÀÏ, ij³ª´Ù, ¸ß½ÃÄÚ, ¹Ì±¹ ÀϺΠÁö¿ª¿¡¼­ °³±â ÀϽÄÀÌ ¹ß»ýÇß½À´Ï´Ù . ÀÌ Çö»óÀº ÇâÈÄ 20³â µ¿¾È ¹ß»ýÇÏÁö ¾ÊÀ» °ÍÀÔ´Ï´Ù.

     



     

     

    The path of totality then continued through the southern US and into the northeast, tracing the border with Canada.

    °³±âÀϽÄÀÇ ±æÀº ¹Ì±¹ ³²ºÎ¸¦ °ÅÃÄ ºÏµ¿ÂÊÀ¸·Î À̾îÁ® ij³ª´Ù ±¹°æÀ» µû¶ó À̾îÁ³½À´Ï´Ù.

     

     

    Those squarely along the center line of the path of totality saw an eclipse that lasted between 3 ¨ö and 4 minutes, according to NASA.

    NASA ¿¡ µû¸£¸é °³±âÀÏ½Ä °æ·ÎÀÇ Á߽ɼ±À» µû¶ó ÀÖ´Â »ç¶÷µéÀº 3ºÐ 30ÃÊ¿¡¼­ 4ºÐ µ¿¾È Áö¼ÓµÈ ÀϽÄÀ» º¸¾Ò½À´Ï´Ù .

     

     

    But a great cue for spectators was when the skies started to darken and turn an eerie gray color, about 15 to 20 minutes before totality.

    ±×·¯³ª °üÁߵ鿡°Ô °¡Àå ÁÁÀº ½ÅÈ£´Â °³±âÀÏ½Ä 15~20ºÐ Àü, ÇÏ´ÃÀÌ ¾îµÎ¿öÁö°í À¸½º½ºÇÑ È¸»öÀ¸·Î º¯Çϱ⠽ÃÀÛÇÏ´Â ¼ø°£À̾ú½À´Ï´Ù.

     

     

    Then, several phases happened in quick succession just before the sun¡¯s light completely disappeared from view.

    ±×·± ´ÙÀ½ žçºûÀÌ ½Ã¾ß¿¡¼­ ¿ÏÀüÈ÷ »ç¶óÁö±â Á÷Àü¿¡ ¿©·¯ ´Ü°è°¡ ºü¸£°Ô ¿¬¼ÓÀûÀ¸·Î ¹ß»ýÇß½À´Ï´Ù.

     

     

    Sky-gazers observed drops of sunlight forming around the moon, known as Baily¡¯s beads, as sunlight streamed over the craters and valleys of the lunar surface. After about 30 seconds to a minute, some of those drops appeared to merge together, creating a glistening ¡°diamond ring¡± effect about a minute before totality.

    ÇÏ´ÃÀ» °üÂûÇÏ´Â »ç¶÷µéÀº ÇÞºûÀÌ ´Þ Ç¥¸éÀÇ ºÐÈ­±¸¿Í °è°î À§·Î È帣¸é¼­ º£Àϸ®ÀÇ ±¸½½·Î ¾Ë·ÁÁø ´Þ ÁÖÀ§¿¡ Çü¼ºµÇ´Â ÇÞºû ¹æ¿ïÀ» °üÂûÇß½À´Ï´Ù. ¾à 30ÃÊ¿¡¼­ 1ºÐ ÈÄ¿¡, ±× ¹æ¿ï Áß ÀϺΰ¡ ÇÕÃÄÁ® ​​Àüü°¡ µÇ±â ¾à 1ºÐ Àü¿¡ ¹Ý¦ÀÌ´Â "´ÙÀ̾Ƹóµå ¹ÝÁö" È¿°ú¸¦ ¸¸µå´Â °Íó·³ º¸¿´½À´Ï´Ù.

     

     

    During totality, the luminous glow belonging to the sun¡¯s corona, or hot outer atmosphere, and its faint light is only visible when the sun¡¯s ultrabright surface is blocked.

    °³±âÀÏ½Ä µ¿¾È žçÀÇ Äڷγª, Áï ¶ß°Å¿î ¿ÜºÎ ´ë±â¿¡ ¼ÓÇÏ´Â ºû³ª´Â ºû°ú ±× Èñ¹ÌÇÑ ºûÀº žçÀÇ ¸Å¿ì ¹àÀº Ç¥¸éÀÌ Â÷´ÜµÉ ¶§¸¸ º¼ ¼ö ÀÖ½À´Ï´Ù.

     

     

    While totality is the main event, a few dots of light were also visible in the sky near the eclipse, belonging to Jupiter, Venus, Mars and the faint light from Saturn.

    °³±âÀϽÄÀÌ ÁÖ¿ä »ç°ÇÀÌÁö¸¸ ÀÏ½Ä ±Ùó Çϴÿ¡´Â ¸ñ¼º, ±Ý¼º, È­¼º, Å伺ÀÇ Èñ¹ÌÇÑ ºû¿¡ ¼ÓÇÏ´Â ¸î °³ÀÇ Á¡±¤µµ º¼ ¼ö ÀÖ½À´Ï´Ù.

     

     

    And during the few moments of totality, local temperatures dropped up to 9 degrees Fahrenheit in some areas.

    ±×¸®°í ÀϺΠÁö¿ª¿¡¼­´Â ¼ø°£ÀûÀ¸·Î ±â¿ÂÀÌ È­¾¾ 9µµ±îÁö ¶³¾îÁö±âµµ Çß½À´Ï´Ù.

     

     

    A solar eclipse occurs when the Sun, the Moon, and Earth are aligned, or in syzygy.

    The Moon, directly between the Sun and Earth, casts a shadow on our planet. If you¡¯re in the dark part of that shadow (the umbra), you¡¯ll see a total eclipse. If you¡¯re in the light part (the penumbra), you¡¯ll see a partial eclipse.

    ÀϽÄÀº žç, ´Þ, Áö±¸°¡ Á¤·ÄµÇ°Å³ª ÇÕÀ쵃 ¶§ ¹ß»ýÇÕ´Ï´Ù.

    žç°ú Áö±¸ »çÀÌ¿¡ ÀÖ´Â ´ÞÀº ¿ì¸® Ç༺¿¡ ±×¸²ÀÚ¸¦ µå¸®¿ó´Ï´Ù. ¸¸¾à ´ç½ÅÀÌ ±× ±×¸²ÀÚÀÇ ¾îµÎ¿î ºÎºÐ¿¡ ÀÖ´Ù¸é, °³±âÀϽÄÀ» º¸°Ô µÉ °ÍÀÔ´Ï´Ù. ¹àÀº ºÎºÐ¿¡ ÀÖÀ¸¸é ºÎºÐ ÀϽÄÀ» º¼ ¼ö ÀÖ½À´Ï´Ù.

     

     

     

     

     

     

     

     



     
    [1][2][3][4][5][6][7][8][9][10]