福衛7號第2組取消 太空中心:仍將發射自製衛星

福衛7號第2組取消 太空中心:仍將發射自製衛星
2017-10-21 01:06聯合報 記者陳宛茜╱即時報導

福衛七號太空模擬圖。翻攝自國家太空中心
福衛七號太空模擬圖。翻攝自國家太空中心

因美國資金無法到位,國家太空中心取消福衛7號第2組的發射計畫。國研院深夜發出新聞稿說明,不執行第2組將會降低全球均勻分布的氣象觀測資料量,影響國際間氣象作業中心與研究單位在全球大氣模式預報準確度及相關研究,但對台灣天氣預報的影響極小福衛七號計畫是福衛三號的後續計畫,任務目標為建立一高可靠度操作型衛星系統,延續福衛三號計畫之掩星氣象觀測任務,原規劃有12 枚任務衛星加上1枚國家太空中心自主研製的衛星,分兩批發射。第1組包含6枚任務衛星,第2組則包括7枚衛星(6枚任務衛星+1枚自主衛星)。兩組衛星分別佈署於高低兩種傾角,以提供更多且密集的氣象觀測資料。

國研院表示,依雙方於2013年5月完成簽署的第一號執行協議書,我方負責系統工程設計及整合、衛星本體發展及衛星操控,美方則負責提供任務酬載、科學酬載、全球地面接收站及發射服務。

國家太空中心經多年努力,雖已建立衛星本體完整本土自製能力,然基於時程及資源的考量,第一組6枚衛星本體委由英國SSTL公司製造,於2015年依約遞交。太空中心於2016年已完成衛星組裝測試及星系系統整合測試,目前6枚衛星皆已備便,存放在太空中心廠房內。

第1組6枚衛星高度550公里,傾角24度,繞行地球一圈約97分鐘;6枚衛星佈署完成後,可提供在南北緯50度間每日約4000 筆資料,資料量約是福衛三號資料量3至4倍,大幅增加台灣在內的低緯度地區氣象資料,對國內天氣預報準確度的提升甚有助益。目前第1組星系預計於

2018年4月以後發射,美方提供的發射載具為Space X的獵鷹重型號(Falcon Heavy)火箭。

第2組星系原規劃軌道高度800公里,傾角72度,每天可收集量測4000點全球的資料,以提供分布更均勻的全球資料。

太空中心指出,第2組美方分攤的經費自2014年起即未能被納入美國總統預算書內,於2017年6月召開福七台美共同指導委員第9次會議中,美方復說明NOAA 於2017年5月所提的2018年度總統預算書內仍未編列第2組的預算;基於美方執行經費取得困難,雙方同意檢討第二組衛星星系的執行方案。經過2個月的協商討論後,雙方共同決定「不執行福衛七號第2組6枚衛星星系」,並同意以備忘錄方式記錄終止第二組星系之決定,備忘錄正式簽署等行政程序於10月完成。

國家太空中心另規劃的1枚自主衛星發展則不受影響,持續執行。該自主衛星(FORMOSAT-7R)為300公斤等級衛星,完全由國內自行研發,搭載國內自製的全球衛星導航系統無線電反射訊號接收儀(GNSS-Reflectometry, GNSS-R),4項衛星關鍵元件與過氧化氫衛星推進模組,展現我國先進的衛星技術。

其所得海洋反射訊號可推算海面風速資料,有助於瞭解颱風結構之發展,並可與第1組星系的掩星資料相互搭配,提升颱風強度與降雨量預測的準確性,降低因劇烈天氣所造成的生命財產與經濟之損失。

太空中心表示,目前已完成衛星關鍵設計,準備進行整合測試。原規劃與第2組一併發射,但由於第2組不執行,FORMOSAT-7R將另外尋求共載發射的機會。

太空星系

小辭典-全球分24個標準時區

小辭典-全球分24個標準時區

2017年10月20日 01:03 中國時報 洪凱音

西元1884年,國際性時間會議在美國華盛頓開會決議,全世界統一標準畫分時區,實行分區計時,稱為標準時間,它以格林威治經線為0度作標準,把西經7.5度到東經7.5度均定為零時區,由零時區分別向東與向西每隔15個經度畫為1個時區,東西各有12個時區,全球合計共有24個標準時區,每向東過1時區則鐘錶撥快1小時,向西則撥慢1小時。

(中國時報)

Einstein’s waves win Nobel Prize in physics

Einstein’s waves win Nobel Prize in physics
By Paul Rincon and Jonathan Amos
BBC Science News , 3 October 2017 , From the section Science & Environment

Nobel laureates in physics 2017Image copyright PA
Image captionWeiss (L) takes half the prize; Thorne (C) and Barish (R) share the other half

The 2017 Nobel prize in physics has been awarded to three US scientists for the detection of gravitational waves.

Rainer Weiss, Kip Thorne and Barry Barish will share the nine million kronor (£831,000) prize.

The ripples were predicted by Albert Einstein and are a fundamental consequence of his General Theory of Relativity.

The winners are members of the Ligo-Virgo observatories, which were responsible for the breakthrough.

The winners join a prestigious list of 204 other Physics laureates recognised since 1901.

Prof Weiss gets half of the prize money, while Barish and Thorne will share the other half.

Gravitational waves describe the stretching and squeezing of space-time that occurs when massive objects accelerate.

The warping of space resulting from the merger of two black holes was initially picked up by the US Ligo laboratory in 2015 – the culmination of a decades-long quest.

Three more examples have been detected since then.


Gravitational waves – Ripples in the fabric of space-time

Black hole artworkImage copyrightIGO/CALTECH/MIT/SONOMA STATE
Image captionArtwork: Two coalescing black holes spinning in a non-aligned fashion
  • Gravitational waves are a prediction of the Theory of General Relativity
  • It took decades to develop the technology to directly detect them
  • They are ripples in the fabric of space-time generated by violent events
  • Accelerating masses will produce waves that propagate at the speed of light
  • Detectable sources ought to include merging black holes and neutron stars
  • Ligo/Virgo fire lasers into long, L-shaped tunnels; the waves disturb the light
  • Detecting the waves opens up the Universe to completely new investigations

Speaking at a press conference, Olga Botner, from the Royal Swedish Academy of Sciences, said: “The first ever observation of a gravitational wave was a milestone – a window on the Universe.”

The US Ligo and European Virgo laboratories were built to detect the very subtle signal produced by these waves.

Even though they are produced by colossal phenomena, such as black holes merging, Einstein himself thought the effect might simply be too small to register by technology.

But the three new laureates led the development of a laser-based system that could reach the sensitivity required to bag a detection.

The result was Ligo, a pair of widely separated facilities in North America: one observatory is based in Washington State, while the other is in Livingston, Louisiana.

The European side of the gravitational wave collaboration is based in Pisa, Italy. On 14 August this year, just after coming online, it sensed the most recent of the four gravitational wave events.

Speaking over the phone at the Nobel announcement in Stockholm, Rainer Weiss said the discovery was the work of about 1,000 people.

He explained: “It’s a dedicated effort that’s been going on for – I hate to tell you – it’s as long as 40 years, of people thinking about this, trying to make a detection and sometimes failing in the early days, then slowly but surely getting the technology together to do it. It’s very, very exciting that it worked out in the end.”

Nonetheless, the Nobel trio’s contribution is also regarded as fundamental.

Weiss set out the strategy that would be needed to make a detection.

Thorne did much of the theoretical work that underpinned the quest.

And Barish, who took over as the second director of Ligo in 1994, is credited with driving through organisational reforms and technology choices that would ultimately prove pivotal in the mission’s success.

SimulationImage copyrightS.OSSOKINE/A.BUONANNO (MPI GRAVITATIONAL PHYSICS)
Image captionA computer simulation of gravitational waves radiating from two merging black holes

The Astronomer Royal, Sir Martin Rees, said the three leaders honoured by the Nobel Committee were “outstanding individuals whose contributions were distinctive and complementary”.

But he added: “Of course, Ligo’s success was owed to literally hundreds of dedicated scientists and engineers. The fact that the Nobel committee refuses to make group awards is causing them increasingly frequent problems – and giving a misleading and unfair impression of how a lot of science is actually done.”

Many commentators had gravitational waves down as a dead cert to win last year, but the Nobel committee has always been fiercely independent in its choices and has made everyone wait 12 months.

Had the prize been awarded last year, it is very likely that the Scottish physicist Ron Drever would have shared it with Weiss and Thorne.

The trio won all the big science prizes – apart from the Nobel – in the immediate aftermath of the first detection in 2015.

But Drever died in March this year and Nobels are generally not awarded posthumously.

The Scotsman developed some of the early laser systems at Glasgow University before taking this knowledge to Caltech in California, which manages the Washington State Ligo facility.

Glasgow remains the UK hub for the big British contribution to Ligo. Its Institute for Gravitational Research designed and built the suspension system that holds the ultra-still mirrors used in the US and Italian labs.

Catherine O’Riordan, interim co-chief executive of the American Institute of Physics (AIP), said: “Weiss, Barish and Thorne led us to the first detection of gravitational waves and laid the foundation for the new and exciting era we officially entered on September 14, 2015 – the era of gravity wave astronomy.”

This is actually the second Nobel prize to involve gravitational waves. In 1993, Americans Russell Alan Hulse and Joseph Hooton Taylor were awarded the physics prize for work that provided indirect evidence for the warping of space.

line break

Previous winners of the Nobel Prize in physics

2016 – David Thouless, Duncan Haldane and Michael Kosterlitz shared the award for their work on rare phases of matter.

2015 – Takaaki Kajita and Arthur McDonald were awarded the prize the discovery that neutrinos switch between different “flavours”.

2014 – Isamu Akasaki, Hiroshi Amano and Shuji Nakamura won the physics Nobel for developing the first blue light-emitting diodes (LEDs).

2013 – Francois Englert and Peter Higgs shared the spoils for formulating the theory of the Higgs boson particle.

2012 – Serge Haroche and David J Wineland were awarded the prize for their work with light and matter.

2011 – The discovery that the expansion of the Universe was acceleratingearned Saul Perlmutter, Brian P Schmidt and Adam Riess the physics prize.

2010 – Andre Geim and Konstantin Novoselov were awarded the prize for their discovery of the “wonder material” graphene.

line break

Follow Paul and Jonathan on Twitter.