Webb kosminis teleskopas beveik paruoštas tyrinėti Saulės sistemą


Webb teleskopas L2 Flyby

James Webb kosminis teleskopas (JWST) yra kitas NASA Didžiosios observatorijos; seka Hablo kosminio teleskopo, Komptono gama spindulių observatorijos, Chandra rentgeno observatorijos ir Spitzerio kosminio teleskopo liniją. JWST sujungia dviejų savo pirmtakų savybes, stebėdamas infraraudonųjų spindulių šviesoje, pavyzdžiui, Spitzerį, su puikia raiška, pavyzdžiui, Hablo. Autoriai: NASA, SkyWorks Digital, Northrop Grumman, STScI

Kaip[{” attribute=””>NASA’s final phases of commissioning its science instruments, the JWST team has also begun working on technical operations of the observatory. While the telescope moves through space, it will constantly find distant stars and galaxies and point at them with incredible precision to acquire images and spectra. However, there are also plans to observe planets and their satellites, asteroids, and comets in our solar system, which move across the background stars of our galaxy. Webb must be able to lock on to these objects and track them precisely enough to obtain images and spectra.

Recently, the Webb team completed the first test to track a moving object. The test confirmed that Webb could conduct moving target science! As we progress through commissioning, we will test other objects moving at various speeds to verify we can study objects with Webb that move throughout the solar system.

Today, we asked Heidi Hammel, Webb interdisciplinary scientist for solar system observations, to tell us about her plans for studying Earth’s nearest neighbors:

“I am really excited about Webb’s upcoming first year of science operations! I lead a team of equally excited astronomers eager to begin downloading data. Webb can detect the faint light of the earliest galaxies, but my team will be observing much closer to home. They will use Webb to unravel some of the mysteries that abound in our own solar system.

“One of the questions I get asked frequently is why we need a powerful telescope like Webb to study our nearby solar system. We planetary scientists use telescopes to complement our in situ missions (missions that we send to fly by, orbit, or land on objects). One example of this is how Hubble was used to find the post-New Horizons mission, Arrokoth. We also use telescopes when we don’t have in situ missions planned – like for the distant ice giants Uranus and Neptune or to make measurements of large populations of objects, such as hundreds of asteroids or Kuiper Belt Objects (small ice worlds beyond the orbits of 6481 Tenzing, named after Tenzing Norgay, the famous Tibetan mountain guide who was one of the first people to reach the summit of Mount Everest. Bryan Holler, at the Space Telescope Science Institute, had a choice of about 40 possible asteroids to test the MT tracking, but, as he told our team: “Since the objects were all virtually identical otherwise, picking the one with a name linked to success seemed like a no-brainer.” We like that sort of thing.

Uranus Webb MIRI Spectroscopy

Uranus is shown within the field of view for MIRI spectroscopy. Credit: Keck image and data of Uranus courtesy L. Sromovsky, Leigh Fletcher

“My role with Webb as an ‘Interdisciplinary Scientist’ means that my program uses all of the capabilities of this forefront telescope! We need all of them to truly understand the solar system (and the universe!).

“Our solar system has far more mysteries than my team had time to solve. Our programs will observe objects across the solar system: We will image the giant planets and Saturn’s rings; explore many Kuiper Belt Objects; analyze the atmosphere of Titan; and much more! There are also other teams planning observations; in its first year, 7% of Webb’s time will be focused on objects within our solar system.

“One exciting and challenging program we plan to do is observe ocean worlds. There’s evidence from the Jupiter’s moon Europa has sporadic plumes of water-rich material. We plan to take high-resolution imagery of Europa to study its surface and search for plume activity and active geologic processes. If we locate a plume, we will use Webb’s spectroscopy to analyze the plume’s composition.

Europa Webb NURSpec Spectroscopy

Simulated spectroscopy results from the plumes of Europa. This is an example of the data the Webb telescope could return that could identify the composition of subsurface ocean of this moon. Credit: NASA-GSFC/SVS, Hubble Space Telescope, Stefanie Milam, Geronimo Villanueva

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