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Project Blue will place a state-of-the-art exoplanet imaging telescope into orbit. The instrument will be equipped with advanced high contrast imaging technologies embedded in a coronagraph with a deformable mirror, multi-star wavefront control, and specialized post-processing techniques. Together they can efficiently suppress the light from both stars (Alpha Centauri A and B) separately, thus allowing any planets to be seen. Our team has extensive experience developing and testing these technologies — now it’s time to get them into space!
Why Alpha Centauri?
Quite simply, we believe Alpha Centauri is the best target for direct imaging an Earth-like planet in coming years.
Unusual proximity: At only 4.37 light years distance, Alpha Centauri is the closest star system to us, and contains not just one, but two stars similar to our Sun. The next Sun-like star is located 2.5x further away and would require a telescope 2.5 times larger in size.*
Accessible Habitable Zone: Its proximity allows us to observe the habitable zone of each star for Earth-like planets with a modest space telescope with a powerful coronagraph, while any other star requires telescopes of at least 1 meter in size.
Fertile ground: Proxima Centauri, which is thought to be part of the same system, is now known to have a potentially habitable planet. We are acting on a new scientific urgency to investigate our nearest Sun-like stars!
Timeline
2016: *Form partnerships & initiate fundraising
2017: * Preliminary design, proof of concept prototypes, integration, and initial instrument prototype
2018: * Final mission design, fabrication, assembly & testing; incorporate lessons learned from related balloon-borne flights
2019: * Final construction and launch to low-Earth orbit
2020 - 2022: Science and mission operations
The movie uses four MAVEN images to show about 7 hours of Mars rotation during this period, and interleaves simulated views that would be seen between the four images. Mars' day is similar to Earth’s, so the movie shows just over a quarter day. The left part of the planet is in morning and the right side in afternoon.
Mars’ prominent volcanoes, topped with white clouds, can be seen moving across the disk. Mars’ tallest volcano, Olympus Mons, appears as a prominent dark region near the top of the images, with a small white cloud at the summit that grows during the day. Olympus Mons appears dark because the volcano rises up above much of the hazy atmosphere which makes the rest of the planet appear lighter.
Three more volcanoes appear in a diagonal row, with their cloud cover merging to span up to a thousand miles by the end of the day.
These images are particularly interesting because they show how rapidly and extensively the clouds topping the volcanoes form in the afternoon. Similar processes occur at Earth, with the flow of winds over mountains creating clouds. Afternoon cloud formation is a common occurrence in the American West, especially during the summer.
The delicate sphere of gas, photographed by NASA's Hubble Space Telescope, is the result of gas that is being shocked by the expanding blast wave from a supernova. The bubble is the visible remnant of a powerful stellar explosion in the Large Magellanic Cloud (LMC), a small galaxy about 160,000 light-years from Earth. Ripples in the shell's surface may be caused by either subtle variations in the density of the ambient interstellar gas, or possibly driven from the interior by pieces of the ejecta. The bubble-shaped shroud of gas is 23 light-years across and is expanding at more than 11 million miles per hour (5,000 kilometers per second).
The unique three-dimensional view of the visualization reminds us that the objects in Hubble images are not all at the same distance, but rather spread across light-years of space. The stars and the shell of glowing gas from the Hubble two-dimensional image have been separated using both scientific knowledge and artistic license to create the depth in the movie. Of note, the relative distances between stars and the nebula have been greatly compressed.
Credit: NASA, ESA, and G. Bacon, T. Borders, L. Frattare, Z. Levay, and F. Summers (STScI)
The telescope was moved via crane to a rotating stand to prep and position it for center of curvature testing. Precise measurements of the mirrors will be done via laser interferometer both before and after environmental testing. (i.e. vibration testing to simulate a rocket launch)
Launched ten years ago, on Oct. 25, 2006, the twin spacecraft of NASA’s STEREO mission – short for Solar and Terrestrial Relations Observatory – have given us unprecedented views of the sun, including the first-ever simultaneous view of the entire star at once. This kind of comprehensive data is key to understanding how the sun erupts with things like coronal mass ejections and energetic particles, as well as how those events move through space, sometimes impacting Earth and other worlds. Ten years ago, the twin STEREO spacecraft joined a fleet of NASA spacecraft monitoring the sun and its influence on Earth and space – and they provided a new and unique perspective.
The two STEREO observatories, called STEREO-A and STEREO-B – for Ahead and Behind, respectively – were sent out from Earth in opposite directions. Using gravitational assists from both the moon and Earth, the STEREO spacecraft were accelerated to Earth-escape velocities.
STEREO-A was inserted into an orbit slightly smaller, and therefore faster, than Earth’s. For STEREO-B, the reverse happened: It was nudged into an orbit slightly larger than Earth’s so that it traveled around the sun more slowly, falling increasingly behind the Earth. As the spacecraft slowly fanned out away from the centerline between Earth and the sun – where every other sun-watching spacecraft is located – they revealed more and more new information about our closest star.