How will NASA’s web telescope continue the legacy of the spitzer’s, When one window to the universe closes, another window opens with an even better view. Some of the planets, stars and galaxies that we first see in the first window are shown in even sharper detail in the next window.
Telescopes make many discoveries beyond the imagination of designers, such as planets outside our solar system, called exoplanets and galaxies, which formed at the beginning of the universe.
Many of Spitzer’s breakthroughs will be explored in more detail with the upcoming James Webb Space Telescope, which is expected to be launched in 2021. now the NASA’s web telescope continue the legacy.
Both Web and Spitzer specialize in infrared light that is not visible to the human eye. But with a large beryllium gold mirror and nine new technologies, Webb is about 1,000 times stronger.
The upcoming telescope will be able to bring Spicer’s scientific breakthrough to new frontiers, from identifying chemicals in the exoplanet’s atmosphere to discovering the first few galaxies formed after the Big Bang. In addition to his invention, Spitzer is also a guide to the Internet about the operation of such a telescope. To measure extremely sensitive infrared light, a telescope must be very cold.
Spitzer showed the engineers how far away the behavior of the infrared observatory and which mission planners were expected from Webb.
Having a giant telescope in space is difficult. But having a cool giant telescope is far more difficult, “said Amber Straun, deputy scientist for the James Communb Communication Science Space Telescope project. Spitzer helped us work better with very cold telescopes in more than 8,700 Scientific reports based on the discovery of the Speaker have made the telescope as a great asset for astronomers in various disciplines, and many of these painful results can be verified with more powerful telescopes and the web is ready to start with its mission.
WASP-18b is another interesting planet that Spitzer has studied, and this web is further examined in observations made at the beginning of the mission. This gas giant, ten times the size of Jupiter, is very close to its star and reaches orbit every 23 hours. Because of its high temperature – 2650 degrees Celsius (4800 degrees Fahrenheit) and its size – it’s called a hot Jupiter. Using data from Spitzer and Hubble, astronomers found in 2017 that the planet contains a lot of carbon monoxide in the upper atmosphere and less water vapor.
This planet is very interesting because it is so close to its star that it is in danger of being torn apart and may not last for millions of more years. Astronomers are interested in using Webb to study the processes in the planet’s atmosphere that give a picture of Jupiter as a whole heat.
Spitzer also gave an unprecedented meteorological report on exoplanets. In 2007, he made the first map of the surface of an extrasolar planet, Jupiter HD 189733b, which showed fluctuations in temperature and cloud tops. Most recently, in 2016 Spitzer showed a climate model of 55 Cancri e, which might be covered with lava and more than twice the size of the earth. But the Spitzer card has given many scientists to think about if they want to do more research on the Internet.
At present it is not possible to determine hundreds of billions of galaxies, but Spitzer has made a large catalog of galaxies that represent various areas in the universe and contain some of the most distant galaxies that we know of. With the Spitzer and Hubble space telescopes with large mirrors, astronomers can effectively look for objects that can be examined closer to Webb.
Scientists have used Spitzer to study LIRG and to get information about star formation and the growth of black holes in the fast evolutionary phase where galaxies collide and unite.
Such collisions are even more common 6 to 10 billion years ago and have influenced the evolution of the universe as we know it. The web will be inspired by Spitzer and will study various LIRGs near and far to learn more about the role of galactic mergers, epidemics of star formation and the growth of supermassive black holes in galaxy evolution over spacetime.