Skip to main content

Euclid dark matter telescope arrives at its destination orbit

The European Space Agency (ESA)’s Euclid space telescope has arrived at its orbit around the sun. Launched from Cape Canaveral on July 1, the telescope is now in at orbit around the sun at the L2 Lagrange point, where it joins other space telescopes such as the James Webb Space Telescope and the Gaia space telescope.

Webb and Gaia welcome Euclid to L2

The video above shows how Euclid will join the other space telescopes and how their orbits relate to each other. Located around 1 million miles from Earth, this complex-looking orbit is often used for space telescopes because of its high level of stability. Maintaining the orbit requires only a small amount of fuel, which is a limited resource for space missions, and it also allows the telescopes to stay on the opposite side of the sun from Earth. This means that the telescopes can face away from both the Earth and the sun, avoiding heat and light interference from these two sources.

Recommended Videos

This is important for missions like Webb as it avoids heat buildup because Webb needs to maintain a very cool operating temperature for its observations in the infrared. Whereas Euclid needs to have a very stable orbit, with no wobbles to introduce interference into its highly detailed observations of distant parts of the universe.

Euclid will be observing distant galaxies to build up a 3D map of all the dark matter in the universe. By determining its location by looking at its gravitational effects, scientists hope to learn more about the nature of dark matter.

Even though Euclid shares the L2 orbit with other space telescopes, there is plenty of room for all of them without risk of a collision. “The region around L2 is big and even though the orbits of these spacecraft seem to cross in the animation, in reality there is plenty of space and a collision can be easily avoided,” ESA writes. “For example, Webb and Gaia are between 400,000 and 1,100,000 km [250,000 and 700,000 miles] apart, depending on where they are in their respective orbits.”

With Euclid now at its destination, the next step of the mission is the commissioning phase in which the instruments are prepared for operations. This will take around three months, then the telescope can begin its science operations.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
Neptune has a dark spot of its own, and it has been imaged from Earth
Neptune observed with the MUSE instrument at ESO’s Very Large Telescope.

While the most famous planetary spot in the solar system would have to be Jupiter's Great Red Spot, an epic storm 10,000 miles wide that has been raging for hundreds of years, other planets are known to host spots of their own as well. That includes Neptune, which had a large dark spot that was first imaged by Voyager 2 when it passed by in the 1980s.

Neptune's spot was named the Great Dark Spot, but when the Hubble Space Telescope tried to image the spot in 1994, it had disappeared. Now, a Neptune spot has been imaged from the ground for the first time, using the European Southern Observatory's Very Large Telescope (VLT).

Read more
Watch a video of an exoplanet orbiting its star — made from 17 years of observations
Artist’s impression of the planet Beta Pictoris b orbiting its star.

It's rare that we get to see exoplanets themselves. Most often, planets in other star systems are too small and too dim to be directly detected, so astronomers infer their presence based on their effects on their host stars. But occasionally, it is possible to image a star directly -- and recently, astronomers managed to create not only an image, but a video of an exoplanet orbiting its star.

17 years of real footage of an exoplanet (Beta Pic b)

Read more
See the incredible first images taken by the dark matter-hunting Euclid telescope
Euclid’s Near-Infrared Spectrometer and Photometer (NISP) instrument is dedicated to measuring the amount of light that galaxies emit at each wavelength. It will image the sky in infrared light (900–2000 nm) to measuring the brightness and intensity of light. This image was taken during commissioning of Euclid to check that the focused instrument worked as expected. This is a raw image taken using NISP’s ‘Y’ filter. Because it is largely unprocessed, some unwanted artefacts remain – for example the cosmic rays that shoot straight across, seen especially in the VIS image. The Euclid Consortium will ultimately turn the longer-exposed survey observations into science-ready images that are artefact-free, more detailed, and razor sharp.

The recently-launched Euclid space telescope just took some of its first images, and the European Space Agency (ESA) has shared them to give a taste of what is to come from this dark matter investigation tool.

Even though they are only preliminary test images, they still give a stunning view of distant galaxies and show what Euclid will be able to produce once it begins its science operations in a few months' time. The aim of the mission is to learn about dark matter and dark energy by creating a 3D map of the dark matter in the universe.

Read more