NASA's Hubble Space Telescope has captured high-quality images of three different space environments: the LH 95 star-forming region and two globular clusters known as Messier 3 and NGC 6426.

美國國家航空暨太空總署 (NASA) 的哈伯太空望遠鏡捕捉到了三個不同太空環境的高品質圖像：LH 95 恆星形成區，以及兩個被稱為 Messier 3 與 NGC 6426 的球狀星團。

The study of LH 95, located in the Large Magellanic Cloud, allows scientists to examine how stars are born. This region contains massive blue giants and about 2,500 young stars. Data shows that the rate at which these stars gather mass decreases as they get older, a process that lasts for several million years. Furthermore, researchers found a very large star that is much younger than the others, which suggests that stars in this area were formed in different groups at different times.

對位於大麥哲倫雲的 LH 95 進行研究，讓科學家能夠觀察恆星是如何誕生的。該區域包含巨大的藍色巨星以及約 2,500 顆年輕恆星。數據顯示，這些恆星增加質量的速度會隨著年齡增長而降低，這一過程持續數百萬年。此外，研究人員發現了一顆比其他恆星年輕得多的巨大恆星，這表明該區域的恆星是在不同時間分批形成的。

In contrast, the study of globular clusters M3 and NGC 6426 helps scientists understand the history of the galaxy. M3 contains many 'variable stars' used to measure distance, as well as 'blue stragglers,' which are stars that grew larger by pulling material from other stars. Because M3 has two different groups of stars, experts believe it may have formed when two separate clusters merged, possibly after a small galaxy was absorbed by the Milky Way.

相反地，對球狀星團 M3 與 NGC 6426 的研究有助於科學家了解星系的歷史。M3 包含許多用於測量距離的「變星」，以及「藍色後起之星」(blue stragglers)，即透過吸收其他恆星物質而變得較大的恆星。由於 M3 擁有兩組不同的恆星，專家認為它可能是由兩個獨立的星團合併而成的，可能發生在一個小星系被銀河系吸收之後。

Finally, NGC 6426 is approximately 13 billion years old and contains very few heavy elements, which reflects the chemical state of the early universe. The discovery of two different chemical groups in this cluster indicates that early supernova explosions released materials that helped create a second generation of stars. These findings are part of a larger project to create a timeline of how the Milky Way evolved.

最後，NGC 6426 約有 130 億年歷史，且含有的重元素極少，反映了早期宇宙的化學狀態。在該星團中發現的兩個不同化學組分表明，早期的超新星爆炸釋放了物質，有助於第二代恆星的形成。這些發現是一個更大計畫的一部分，旨在建立銀河系演化的時間線。

These results emphasize how useful Hubble's observations are for mapping both the birth of new stars in LH 95 and the ancient history stored within globular clusters.

這些結果強調了哈伯的觀測在描繪 LH 95 新恆星誕生以及球狀星團中儲存的遠古歷史方面具有極高價值。