ئه‌ستێره‌كانی هاوڕێم

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Showcased at the centre of this NASA/ESA Hubble Space Telescope image is an emission-line star known as IRAS 12196-6300. Located just under 2300 light-years from Earth, this star displays prominent emission lines, meaning that the star’s light, dispersed into a spectrum, shows up as a rainbow of colours marked with a characteristic pattern of dark and bright lines. The characteristics of these lines, when compared to the “fingerprints” left by particular atoms and molecules, can be used to reveal IRAS 12196-6300’s chemical composition. Under 10 million years old and not yet burning hydrogen at its core, unlike the Sun, this star is still in its infancy. Further evidence of IRAS 12196-6300’s youth is provided by the presence of reflection nebulae. These hazy clouds, pictured floating above and below IRAS 12196-6300, are created when light from a star reflects off a high concentration of nearby dust, such as the dusty material still remaining from IRAS 12196-6300’s formation.
هۆنراوە بۆ منداڵان
                  هۆنراوەی: عه‌لی حه‌مه‌ڕه‌شید به‌رزنجی
ئه‌ستێره‌كانی هاوڕێم
هه‌رگیز به‌شه‌و ناخه‌ون
هه‌ر تاریكایی داهات
ئه‌وانیش ده‌رده‌كه‌ون
* * *
حه‌ز ده‌كه‌ن پێكه‌وه‌ بن
تاریكایی ڕاوبنێن
تا به‌یانی گۆرانی
بۆ پرشنگی خۆر بڵێن
* * *
كه‌ خۆر هه‌ڵهات ئه‌وانیش
ده‌ڕۆن و دیار نامێنن
چه‌پك چه‌پك تیشكی گه‌ش
له‌ ناخیاندا ده‌ڕوێنن
* * *
له‌ ئاسمانی به‌رینا
به‌ تیشكه‌وه‌ گه‌شت ده‌كه‌ن
تاریكایی له‌ كوێ‌ بێ
ڕوناكایی بۆ ده‌به‌ن
* * *
چونكه‌ ئه‌ستێره‌كانیش
هه‌روه‌كو ئێمه‌ جوانن
هاوڕێی ئازیزی ئێمه‌ن
هه‌رچه‌نده‌ له‌ ئاسمانن

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