Clearly, as telescopes get bigger their ability to show us faint objects increases enormously.

显然，随着望远镜变得越来越大，它们向我们展示模糊物体的能力也大大增强。

And also it's not really big enough to see those extremely faint objects.

而且它还不够大，看不到那些极其微弱的物体。

The faintest objects in this image are ten billion times dimmer than we can see with our own eyes.

这张图片中最微弱的物体比我们肉眼看到的要暗一百亿倍。

They then let it stare, simply collecting light from whatever it could see, letting light accumulate until incredibly faint objects could be detected.

然后，他们将它对准一个地方，简单地收集它所能看到的光线，让光线不断累积，直到能探测到极其微弱的物体。

This, though, does not affect the system's optical properties and it can, indeed, see small, faint objects that are near large, bright ones.

尽管如此，这并不影响整个系统的视觉特性，并且，它也确实能够看见巨大且明亮的恒星旁边那些小型且微弱的物体。

It also means we can loft telescopes into space, above the sea of air in our atmosphere that blurs and distorts distant, faint objects.

这也意味着我们可以将望远镜架设到太空中，处于会使遥远或暗淡的物体更模糊的大气层之上。

Bigger telescope mirrors let us take sharper and clearer images, and they also make it easier for us to gather light from faint and faraway objects.

更大的望远镜镜子让我们拍摄出更锐利、更清晰的图像，它们也让我们更容易从微弱和遥远的物体中收集光线。

They help us resolve the details of fainter objects like stars and Galaxies that were born much closer to the Big Bang than some of the other ones that perhaps Hubble can see.

这些信息可以帮助我们了解暗物质的细节，如恒星和银河系。相较于哈勃望远镜观察到的星体，它们的诞生时间更接近宇宙大爆炸。

Acting a bit like a lens for a camera, Vantablack basically prevents lens glass in powerful telescope, reducing that stray light allows us to see some of the faintest, and most distant objects in the universe.

就像摄像机的镜头一样。纳米碳管黑体可以防止望远镜镜片上的光散射，以便我们能看到，宇宙中最微弱最遥远物体上的光。