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How The Universe Works is a science documentary television series that provides scientific explanations about the inner workings ... to the vast cosmos seen today. ...
It appears to be expanding faster today than it did in the past. For years, scientists have been troubled by an unusual feature of our universe. It appears to be expanding faster today than it did ...
The universe also has vast regions of relative emptiness; the largest known void measures 1.8 billion ly (550 Mpc) across. [114] Comparison of the contents of the universe today to 380,000 years after the Big Bang, as measured with 5 year WMAP data (from 2008). [115] Due to rounding, the sum of these numbers is not 100%.
Thaller is a regular contributor to the online edition of the Christian Science Monitor, for which she writes a monthly science column, [6] [8] and appears on the History Channel show, The Universe, and The Science Channel series How the Universe Works, Strip the Cosmos, and The Planets and Beyond.
Oluseyi appears as a commentator and scientific authority on Science Channel television shows including How the Universe Works, Outrageous Acts of Science, Curiosity, NASA's Unexplained Files, Space's Deepest Secrets, and Strip the Cosmos,. [26] He also appeared as a 'bakineering' (baking and engineering) judge on Netflix's Baking Impossible.
The history of the universe after inflation but before a time of about 1 second is largely unknown. [26] However, the universe is known to have been dominated by ultrarelativistic Standard Model particles, conventionally called radiation, by the time of neutrino decoupling at about 1 second. [27]
She does science outreach through her work as an expert contributor to the Science/Discovery program How the Universe Works and other television and radio programs. In December 2012, Radebaugh and her colleagues on the Cassini mission announced the discovery of Vid Flumina , a liquid methane river on Saturn's moon Titan over 320 km (200 mi ...
The universe will become extremely dark after the last stars burn out. Even so, there can still be occasional light in the universe. One of the ways the universe can be illuminated is if two carbon–oxygen white dwarfs with a combined mass of more than the Chandrasekhar limit of about 1.4 solar masses happen