求翻译帝，速度进

刚收到的E-MAIL，谁来帮我翻译下啊

We are writing to announce the launch of Phase 3 of Stardust@home.

All dusters are familiar with the words that appear when starting a dusting session: "Expect the unexpected." The unexpected has certainly happened. We are cautiously excited about an interstellar dust candidate, named Orion by its discoverer, Bruce Hudson from Ontario, Canada. This particle is a so-called "midnight" track, because of the angle of its direction on entry into the collector, and looks quite different from our original expectations about what an interstellar dust track might look like. But synchrotron analyses of this particle indicate that it may be the first known sample of matter ever collected from the local interstellar medium.  

So far, Orion is unique. We are desperate to find more midnight tracks. To learn more, see the ISPE Update #6 <http://stardustathome.ssl.berkeley.edu/ISPE_update/#six&gt;.

We expect to launch Phase 3 on March 22. The calibration movies in Phase 3 reflect this new direction in finding more midnight tracks. Although we don't insist on it, we encourage you to go through the new  training session, even if you are a very experienced duster. There is no need to re-register.

Your efforts led to the discovery of candidate Orion. It also may be a false alarm, but we are convinced that we are on the right track based on this discovery and recent experiments that we've done with our colleagues at the van de Graaf dust accelerator at Heidelberg.  We are optimistic that during Phase 3 you will find more "midnight" tracks. To be frank, the Stardust@home distributed thinking project was initially met with skepticism by the professional meteoritics community, but the demonstrated success of this approach -- you have discovered 28 tracks that could not have been found by any other means -- has convinced the critics. Congratulations!

Best,

Andrew Westphal
Stardust@home Director              
Senior Fellow and Associate Director
Space Sciences Laboratory
University of California at Berkeley

==============================================================================================
Disclaimer:  You are receiving this e-mail because you registered on the Stardust@home
website.  If you would prefer to receive no further e-mails from Stardust@home please visit
http://stardustathome.ssl.berkeley.edu after we have come back up, probably on March 22,
login and change your e-mail preference under "My Account" to opt out of e-mail updates.

Please do not reply to this e-mail address -- it does not accept incoming e-mails.
Our physical address is:  
Stardust@home
Space Sciences Laboratory
7 Gauss Way
Berkeley, CA 94720-7450
USA

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我们写这封信，公布了第3期星尘@家推出。



所有的抹布熟悉的话，那启动时出现扬尘会议：“非常意外。”意外的确实发生了。我们审慎兴奋的星际尘埃的候选人，其发现者命名猎户座，布鲁斯哈德森从加拿大安大略省。这种粒子是一个所谓的“午夜”的轨道，由于其对收集到进入方向的角度，并期待什么很大的星际尘埃的轨道可能看起来像我们原来的期望不同。但是，这种粒子同步分析表明，它可能是第一个已知的物质样本都从本地星际介质收集。



到目前为止，猎户座是独一无二的。我们迫切希望找到更多的午夜轨道。要了解更多信息，请ISPE在更新＃6 <http://stardustathome.ssl.berkeley.edu/ISPE_update/#six>。



我们希望可以在3月22日第3期。在第三阶段的校准电影反映在寻找新的方向多米

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