Recent developments in astronomy have made it possible to detect planets in our own Milky Way and in other galaxies. This is a major achievement because, in relative terms, planets are very small and do not emit light. Finding planets is proving hard enough, but finding life on them will prove infinitely more difficult. The first question to answer is whether a planet can actually support life. In our own solar system, for example, Venus is far too hot and Mars is far too cold to support life. Only the Earth provides ideal conditions, and even here it has taken more than 4 billion years for plant and animal life to evolve.

Whether a planet can support life depends on the size and brightness of its star, that is its 'sun'. Imagine a star up to 20 times larger, brighter and hotter than our own sun. A planet would have to be a very long way from it to be capable of supporting life. Alternatively, if the star were small, the life-supporting planet would have to have a close orbit round it and also provide the perfect conditions for life forms to develop. But how would we find such a planet? At present, there is no telescope in existence that is capable of detecting the presence of life. The development of such a telescope will be one of the great astronomical projects of the 21st century.

It is impossible to look for life on another planet using earth-based telescopes. Our own warm atmosphere and the heat generated by the telescope would make it impossible to detect objects as small as planets. Even a telescope in orbit round the earth, like the very successful Hubble telescope, would not be suitable because of the dust particles in our solar system. A telescope would have to be as far away as the planet Jupiter to look for life in outer space, because the dust becomes thinner the further we travel towards the outer edges of our own solar system. Once we detected a planet, we would have to find a way of blotting out the light from its star, so that we would be able to 'see' the planet properly and analyze its atmosphere. In the first instance, we would be looking for plant life, rather than 'little green men'. The life forms most likely to develop on a planet would be bacteria. It is bacteria that have generated the oxygen we breathe on earth. For most of the earth's history they have been the only form of life on our planet. As Earth-dwellers, we always cherish the hope that we will be visited by little green men and that we will be able to communicate with them. But this hope is always in the realms of science fiction. If we were able to discover lowly forms of life like bacteria on another planet, it would completely change our view of ourselves. As Daniel Goldin of NASA observed, 'Finding life elsewhere would change everything. No human endeavour or thought would be unchanged by it.'

New words and expressions 生詞與短語(yǔ)

astronomy

n. 天文學(xué)

relative

adj. 相對(duì)的

infinitely

adv. 無(wú)限地，無(wú)窮地

solar

adj. 太陽(yáng)系的

Venus

n. 金星

Mars

n. 火星

orbit

n. 運(yùn)行軌道

astronomical

adj. 天文學(xué)的

generate

v. 產(chǎn)生

particle

n. 微粒，粒子

Jupiter

n. 木星

blot

v. 遮暗

analyse

v. 分析

bacteria

n. 細(xì)菌

oxygen

n. 氧氣

realm

n. 領(lǐng)域

endeavour

v. 努力

本文參考譯文

天文學(xué)方面最新發(fā)展使得我們能夠在銀河系和其他星系發(fā)現(xiàn)行星。這是一個(gè)重要的成就，因?yàn)橄鄬?duì)來(lái)說(shuō)，行星很小，而且也不發(fā)光。尋找行星證明相當(dāng)困難，但是要在行星上發(fā)現(xiàn)生命會(huì)變得無(wú)比艱難。第一個(gè)需要解答的問(wèn)題是一顆行星是否有能夠維持生命的條件。舉例來(lái)說(shuō)，在我們的太陽(yáng)系里，對(duì)于生命來(lái)說(shuō)，金星的溫度太高，而火星的溫度則太低。只有地球提供理想的條件，而即使在這里，植物和動(dòng)物的進(jìn)化也用了40億年的時(shí)間。

一顆行星是否能夠維持生命取決于它的恒星——即它的“太陽(yáng)”——的大小和亮度。設(shè)想一下，一顆恒星比我們的太陽(yáng)還要大，還要亮，還要熱20倍，那么一顆行星為了維持生命就要離開(kāi)的它的恒星非常遠(yuǎn)。反之，如果恒星很小，維持生命的行星就要在離恒星很近的軌道上運(yùn)行，而且要有極好的條件才能使生命得以發(fā)展，但是，我們?nèi)绾尾拍苷业竭@樣一顆行星呢?現(xiàn)在，沒(méi)有一臺(tái)現(xiàn)存的望遠(yuǎn)鏡可以發(fā)現(xiàn)生命的存在。而開(kāi)發(fā)這樣一臺(tái)望遠(yuǎn)鏡將會(huì)是21世紀(jì)天文學(xué)的一個(gè)重要的研究課題。

使用放置在地球上的望遠(yuǎn)鏡是無(wú)法觀察到其他行星的生命的。地球周?chē)鷾嘏�的大氣層和望遠(yuǎn)鏡散出的熱量使得我們根本不可能找到比行星更小的物體。即使是一臺(tái)放置在圍繞地球的軌道上的望遠(yuǎn)鏡——如非常成功的哈勃望遠(yuǎn)鏡——也因?yàn)樘��?yáng)系中的塵埃微粒而無(wú)法勝任。望遠(yuǎn)鏡要放置在木星那樣遙遠(yuǎn)的行星上才有可能在外層空間搜尋生命。因?yàn)槲覀冊(cè)绞墙咏�太�?yáng)系的邊緣，塵埃就越稀薄。一旦我們找到這樣一顆行星，我們就要想辦法將它的恒星射過(guò)來(lái)的光線遮暗，這樣我們就能徹底“看見(jiàn)”這顆行星，并分析它的大氣層。首先我們要尋找植物，而不是那種“小綠人”。行星上最容易生存下來(lái)的是細(xì)菌。正是細(xì)菌生產(chǎn)出我們?cè)诘厍蛏虾粑�的氧氣。在地球上發(fā)展的大部分進(jìn)程中，細(xì)菌是地球上唯一的生命形式。作為地球上的居民，我們總存有這樣的希望：小綠人來(lái)拜訪我們，而我們可以和他們交流。但是，這種希望總是只在科幻小說(shuō)中存在。如果我們能夠在另一顆行星上找到諸如細(xì)菌的那種低等生命，那么這個(gè)發(fā)現(xiàn)將徹底改變我們對(duì)我們自己的看法。正如美國(guó)國(guó)家航空和宇宙航空局的丹尼爾.戈?duì)柖≈赋龅?ldquo;在其他地方發(fā)現(xiàn)生命會(huì)改變一切。任何人類的努力和想法都會(huì)發(fā)生變化。

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