That's because the sun is eight light-minutes away from earth. When you look at the sunrise or sunset, you are actually seeing the sun as it appeared eight minutes ago. What few people know is, looking into space is also looking back in time. But after decades of development, we are now capable of launching a telescope that is so powerful, it will look back to the beginning of time. Until now, the technology and budget to achieve this was out of reach. From there, the telescope will unfold and begin exploring the cosmos, on a mission to answer some remarkably profound questions about our universe. The rocket will loft the James Webb Space Telescope on a complex trajectory, and if all goes well, it will park the massive satellite behind the Moon. LOS ANGELES, CA (California Network) - On December 22, a rocket will lift off from a pad in French Guiana. We are constantly trying to develop bigger and better telescopes to see farther away (farther back in time), closer to the beginning of the universe, that point in time when God said fiat lux (’let there be light’).Keywords: James Webb Space Telescope, creation, God, time Hence they are looking at history or back in time. When astronomers view an object 3000 light years away, they are looking at light that left that celestial object 3000 years ago. Astronomers actually use the time it takes light to travel as a distance measurement - a light year, the distance light travels in one year (about 6 trillion miles). We do not know what is actually happening there now. Thus, when we observe this star we are seeing it as it was 4.3 years ago. Light from that star takes 4.3 years to reach us. Light from nearby stars take less time to travel to Earth than light from distant stars.Īfter the Sun, the next closest star, Proxima Centauri, is 25 trillion miles from Earth. On any given day you can read yesterday's news in the paper you received from Memphis but the news in the San Francisco paper is five days old. The paper from San Francisco will be older than the paper from Memphis since it has taken longer to get here. When you receive the papers every day, each copy will be a few days old. The papers all travel by trucks going 60 mph. Perhaps as a more obvious example, assume three friends send you a local newspaper every day one lives in Memphis, one in Denver, and one in San Francisco. (Actually 93 million miles divided by 186 000 mps is 500 seconds or a little over 8 minutes.) Thus, we are actually perceiving what happened on the Sun 8 minutes ago. When we look at sunlight, the light that we receive was emitted from the Sun a few minutes ago. For example, the Sun is 93 million miles away. If we know the distance to the point of origin, we can calculate the time it takes that light to get to Earth. Light travels at a specific speed in space (186 000 miles per second). When observing through a telescope, we are seeing light that left some place in the past. If we know the speed of the object, then the time can be calculated by dividing the distance by that speed. Using this relationship we can ask how long something takes to travel a certain distance. In science, speed is equal to the distance traveled divided by the time traveled. To answer this question we must turn to a relationship of science that involves the basic concepts of space (distance) and time, and ties them together through a term called speed. The millions of dollars spent on the COBE project were intended to accomplish one thing - to take baby pictures of the Universe, to look back in time, and see the universe as it was a very long time ago. After a series of tests, COBE’s cryocooled infrared and microwave sensors were deployed to snap photos of the universe. Then the booster, Atlas rocket 189, ejected COBE and the satellite’s two solar panels unfurled like the wings on an insect. The Cosmic Background Explorer satellite (COBE) was thrust into space atop a pillar of fire. Why do astronomers say that when we look at the sky, we are looking backward in time? June 2000 Vocatio Center for Life Calling and Career.Office of Student Leadership & Engagement.
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