Essentially all young stars have these disks, so we expect that these young stars at least have the possibility of having planetary systems.
哈勃”所拍摄的目标为一群名为“R136”的年轻恒星,它们的年龄只有几百万.
Young stellar grouping, called R136, is only a few million years old.
金牛T星是质量低于2.5M☉的年轻恒星,显示出较活跃的活动。
The T Tauri stars are young stars with mass less than about 2.5 M☉ showing a heightened level of activity.
一颗高速移动的年轻恒星与气体和尘埃云的交互作用,可能生成这个具有罕见锐边的明亮弧形。
The interaction of a high velocity young star and the cloud of gas and dust may have created this unusually sharp-edged bright arc.
环中的气体被转换成热的年轻恒星,然后将灰尘加热,使其发出红外光。
Gas in the ring is being converted into hot, young stars, which then warm the dust, causing it to glow with infrared light.
当我们确认这一发现时,我们感到非常兴奋,因为这颗行星围绕着这样一个明亮的,着名的年轻恒星运转。
So we were really excited when we confirmed this discovery because the planet orbits such a bright,well-known young star.”.
在其他模糊的尘埃云靠近热的年轻恒星的地方,它们也反射星光,形成蓝色反射星云。
Where the otherwise obscuringdust clouds lie close to the hot, young stars they also reflect starlight, forming blue reflection nebulae.
在它的外侧边缘,有一个年龄在500万年的年轻恒星团NGC602。
Near its outskirts lies a 5 million year young star cluster called NGC 602.
与之形成鲜明对比的是蓝色反射星云NGC2023,它环绕着一颗炽热的年轻恒星,位于这幅影像的左下方。
Contrasting blue reflection nebula NGC 2023,surrounding a hot, young star, is at the lower left.
猎户星云的年轻恒星仅约1百万岁,和太阳46亿岁的年龄比较。
Orion's young stars are only about 1 million years old, compared to the Sun's age of 4.6 billion years.
猎户座的年轻恒星只有大约100万年的历史,而太阳的年龄是46亿年。
Orion's young stars are only about 1 million years old, compared to the Sun's age of 4.6 billion years.
一颗新发现的行星围绕着已知的最亮的年轻恒星之一,可以提供有关行星体如何形成的宝贵信息。
A newly-discovered planet orbiting one of the brightest young stars known could provide valuable information on how planetary bodies form.
它的蓝色色调是由于灰尘优先反映了该地区炎热的年轻恒星的蓝光。
Its blue tint is due to dustpreferentially reflecting the blue light of hot, young stars in the region.
这些戏剧性的对象是活跃的恒星形成区域,炽热的年轻恒星,导致周围的氢气辉光红色。
These dramatic objects are regions ofactive star formation where the hot young stars are causing the surrounding hydrogen gas to glow red.
这些新的图像刺穿了朦胧,揭示了新的原恒星或胚胎星以及以前从未见过的年轻恒星的诞生。
These new images pierce through the obscuration to reveal the birth of new protostars,or embryonic stars, and young stars never before seen.
这一合并引发了新恒星形成的爆发,并引发了许多炽热的年轻恒星以超新星的形式爆炸。
This merger sparked bursts of new star formation andtriggered many hot young stars to explode as supernovae.
哈勃和其他望远镜的观测结果表明,环形或球形分布的冰碎片环绕着正在形成行星的年轻恒星。
Observations by Hubble and other telescopes have revealed that shells andrings of icy fragments encompass young stars where planet formation is ongoing.
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