{"id":111,"date":"2010-09-27T15:36:52","date_gmt":"2010-09-27T07:36:52","guid":{"rendered":"http:\/\/stuif.com\/blog\/?p=111"},"modified":"2012-09-14T15:38:14","modified_gmt":"2012-09-14T07:38:14","slug":"the-great-debate-are-we-alone-part-1","status":"publish","type":"post","link":"https:\/\/stuif.com\/blog\/?p=111","title":{"rendered":"The Great Debate: Are we alone? part 1"},"content":{"rendered":"

On 26 April 1920, a debate took place at the Smithsonian Museum of Natural History (Washington DC), between two American astronomers, Shapley and Curtis, about the scale of the Universe. Point of contention was the distance of the “nebulae” like Andromeda.
\nShapley argued that the Milky Way was the entirety of the Universe and the Andromeda nebula was inside the Milky Way.
\nCurtis contended that Andromeda and other nebulae were separate island galaxies.
\nThe debate became known later as The Great Debate<\/a>.
\nWe know now that Curtis was right. The Universe is huge and our Milky Way is only one of ~ 100 billion galaxies. Each galaxy contains on average 100 billion stars.
\nOur Sun is one of these ~ 10.000.000.000.000.000.000.000 (!) stars, and was formed relatively recently, about 4.6 billion years ago (The Universe is ~ 13.8 billion years old)
\nEight planets orbit the Sun (sorry for Pluto, not a planet anymore…), and on (only?) one of them, our beautiful Earth, life developed, about 4 billion years ago.
\nEvolution took place. But it was only about 200.000(!) years ago that Homo Sapiens (yes, that’s us) evolved, most probably in Africa<\/a>.<\/p>\n

\"\"<\/a><\/p>\n

Was that a unique incident?<\/p>\n

About half a year ago another astronomical debate took place, at Berkeley University, 30 April 2010, almost exactly 90 years later, and it was also called a Great Debate<\/strong>.
\nA bit preposterous, IMHO…:-)
\nThis time the topic was: Are we alone in the Universe?<\/strong><\/span>
\nThe recording of the debate can be viewed at http:\/\/seti.berkeley.edu\/the-great-debate<\/a> . Be warned, it takes 1.5 hours…:-), but watching it is worthwhile…<\/p>\n

Debaters were Dan Werthimer<\/a>, the chief scientist of the SETI<\/a> project, and Jeff Marcy<\/a>, an astronomer who has discovered more extrasolar planets<\/a> than anyone else.<\/p>\n

The SETI project is S<\/strong><\/span>earching for E<\/strong><\/span>xtra T<\/strong><\/span>errestrial I<\/strong><\/span>ntelligence, so Werthimer is, not surprisingly, convinced that there are many planets with highly developed technological civilizations around us. SETI is searching for about 40 years now ‘only’, it will just take more time to find evidence for intelligent life elsewhere in the Universe, according to him.<\/p>\n

Marcy is a skeptic. Ok, many, if not most, stars will have planets orbiting around them. And he agrees with Werthimer that primitive life will be “teeming” in the Universe.
\nBut intelligent life? Is that an evolutionary advantage? The dinosaurs ruled the world for 200 million years and never developed intelligence with their peanut brains! Why not?
\nMaybe speed or a thick skull will serve you better to survive. Maybe we humans are just a freak evolutionary incident?<\/p>\n

He has other interesting arguments. For example the water content of a planet. Quite critical.
\nAssuming that water has been brought to the earth by asteroids, it should be about 0.03%. Not more, nor less.
\nLess, and the planet will be a desert. More, and it will be just oceans. Is a technological civilisation possible under those adverse conditions?<\/p>\n

At the end of the debate, after a Q&A session, there is a poll for the audience. Are we alone or not?<\/p>\n

I have an opinion myself, but will only tell you in the second part of this email…:-)<\/p>\n","protected":false},"excerpt":{"rendered":"

On 26 April 1920, a debate took place at the Smithsonian Museum of Natural History (Washington DC), between two American astronomers, Shapley and Curtis, about the scale of the Universe. Point of contention was the distance of the “nebulae” like … Continue reading →<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_jetpack_memberships_contains_paid_content":false,"footnotes":"","jetpack_publicize_message":"","jetpack_publicize_feature_enabled":true,"jetpack_social_post_already_shared":false,"jetpack_social_options":{"image_generator_settings":{"template":"highway","enabled":false},"version":2}},"categories":[10,9,7],"tags":[],"class_list":["post-111","post","type-post","status-publish","format-standard","hentry","category-cosmology","category-evolution","category-science"],"jetpack_publicize_connections":[],"jetpack_featured_media_url":"","jetpack_shortlink":"https:\/\/wp.me\/p2LqIR-1N","jetpack_sharing_enabled":true,"_links":{"self":[{"href":"https:\/\/stuif.com\/blog\/index.php?rest_route=\/wp\/v2\/posts\/111","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/stuif.com\/blog\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/stuif.com\/blog\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/stuif.com\/blog\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/stuif.com\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=111"}],"version-history":[{"count":3,"href":"https:\/\/stuif.com\/blog\/index.php?rest_route=\/wp\/v2\/posts\/111\/revisions"}],"predecessor-version":[{"id":116,"href":"https:\/\/stuif.com\/blog\/index.php?rest_route=\/wp\/v2\/posts\/111\/revisions\/116"}],"wp:attachment":[{"href":"https:\/\/stuif.com\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=111"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/stuif.com\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=111"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/stuif.com\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=111"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}