Astronomers from NASA (National Aeronautics and Space Administration) for the first time have discovered seven new Earth-sized exoplanets that may be able to sustain life. The planets were detected using NASA’s Spitzer Space Telescope and several ground-based observatories including Trappist robotic telescope at La Silla, Chile. A huddle of seven worlds, all close in size to Earth, and perhaps warm enough for water and the life it can sustain, has been spotted around a small, faint star in the constellation of Aquarius. The discovery, which has thrilled astronomers, has raised hopes that the hunt for alien life beyond the solar system could start much sooner than previously thought, with the next generation of telescopes that are due to switch on in the next decade. It is the first time that so many Earth-sized planets have been found in orbit around the same star, an unexpected haul that suggests the Milky Way may be teeming with worlds that, in size and firmness underfoot at least, resemble our own rocky home. The planets closely circle a dwarf star named Trappist-1, which at 39 light years away makes the system a prime candidate to search for signs of life. Only marginally larger than Jupiter, the star shines with a feeble light about 2,000 times fainter than our sun. The star is so small and cold that the seven planets are temperate, which means that they could have some liquid water and maybe life, by extension, on the surface. While the planets have Earth-like dimensions, their sizes ranging from 25% smaller to 10% larger, they could not be more different in other features. Most striking is how compact the planet’s orbits are. Mercury, the innermost planet in the solar system, is six times farther from the sun than the outermost seventh planet is from Trappist-1. The discovery prompted more sustained observations from the ground and space. Nasa’s Spitzer space telescope peered at the star for 21 days and, with data from other observatories, revealed a total of seven planets circling Trappist-1. The size of each planet was deduced from the amount of starlight it blocked out, while the mass was estimated from the way it was pushed and pulled around by other planets in the system. The planets are on such tight orbits that it takes between 1.5 and 20 days for them to whip around the star. At such proximity, most, if not all, will be “tidally locked”, meaning they show only one face to Trappist-1, just as one side of the moon always faces Earth. Some of the planets are thought to be the right temperature to host oceans of water, depending on the makeup of their atmospheres, but on others any hospitable regions may be confined to the bands that separate the light and dark sides of the planets.