...the who's who,
and the what's what 
of the space industry

Space Careers

news Space News

Search News Archive

Title

Article text

Keyword

Copernical Team

Copernical Team

Write a comment
Webb telescope's coldest instrument reaches operating temperature
In this illustration, the multilayered sunshield on NASA's James Webb Space Telescope stretches out beneath the observatory's honeycomb mirror. The sunshield is the first step in cooling down Webb's infrared instruments, but the Mid-Infrared Instrument (MIRI) requires additional help to reach its operating temperature. Credit: NASA GSFC/CIL/Adriana Manrique Gutierrez

NASA's James Webb Space Telescope will see the first galaxies to form after the Big Bang, but to do that, its instruments first need to get cold—really cold. On April 7, Webb's Mid-Infrared Instrument (MIRI)—a joint development by NASA and ESA (European Space Agency)—reached its final operating temperature below 7 kelvins (minus 447 degrees Fahrenheit, or minus 266 degrees Celsius).

Write a comment
Concurrent Design Facility

ESA has a new tool for designing space missions. The Agency’s Concurrent Design Facility – bringing together different experts for the rapid creation and evaluation of virtual spacecraft designs – has adopted an advanced software tool, COMET, which will help extend the use of digital models into further mission development phases. Its open source nature means it is freely available beyond ESA Member States, facilitating international cooperation with wider space agencies, research institutions or companies.

Write a comment
Video: 01:15:00

ESA Director General Josef Aschbacher shares the outcome of the ESA Council extraordinary meeting in this virtual Q&A with journalists. Additional updates are provided on ESA’s main programmes, the overall rollout of Agenda 2025 on the way to the ESA Ministerial Meeting in November 2022 as well as further implications of the current geopolitical situation on ESA’s activities.

Write a comment
Tiny but precise: NASA-sponsored team creates compact device to help spaceships land safely on planets
Left: Image of the Fabry-Perot LiDAR. Right: A representation of the whispering gallery mode (WGM) optical microresonator and how it would work. Credit: Elie R. Salameh, Southern Methodist University (SMU)

A NASA-funded team led by SMU researchers think that their small, lightweight device developed to measure spaceship velocity will improve the odds of successful landings on Mars and other planets.

Smaller, they say, is better in space.

The optical microresonator built by the team is only 2 millimeters in length, compared to the velocity-monitoring tool most commonly used on spacecraft—the Fabry-Perot interferometer—which can be as long as 500 millimeters. NASA and other space agencies may be able to use the microresonator to get an accurate, quick measurement of how fast a spaceship is moving in a specific direction.

Write a comment
Radio eye on tree-counting Biomass
Credit: ESA-SJM Photography

The largest antenna ever tested in ESA's Hertz radio frequency test chamber is this 5-m diameter transponder antenna, which will operate down on the ground to help calibrate the Biomass mission, which will chart all the forests on Earth.

"This is a particularly challenging test campaign both in terms of the size of the and the very low P-band frequency that Biomass will be using, which allows it to pierce through forest canopies to acquire individual trees," explains ESA antenna engineer Luis Rolo, overseeing the test campaign.

"Usually when we test a large satellite here, its antenna is significantly smaller, typically between 0.5 and 2 meters across. But this entire structure is a radiating antenna in its own right, its sides coming near to the walls.

"What this means is that the testing process highlight some aspects of the chamber we've never seen before, even after many years of testing. But we've come up with a involving multiple acquisitions from different spots within the chamber, combined carefully to subtract such environmental effects, yielding very accurate results.

Write a comment
Axiom Mission 1 at Pad 39A and Artemis I at Pad 39B
Credit: NASA/Jamie Peer

Axiom Mission 1 (Ax-1) is in the foreground on Launch Pad 39A with NASA's Artemis I in the background on Launch Pad 39B on April 6, 2022.

This is the first time two totally different types of rockets and spacecraft designed to carry humans are on the sister pads at the same time—but it won't be the last as NASA's Kennedy Space Center in Florida continues to grow as a multi-user spaceport to launch both government and commercial rockets.

Ax-1 liftoff is scheduled at 11:17 a.m. EDT Friday, April 8, from Launch Complex 39A at NASA's Kennedy Space Center in Florida.



Citation: Image: Axiom Mission 1 at Pad 39A and Artemis I at Pad 39B (2022, April 13) retrieved 13 April 2022 from https://phys.org/news/2022-04-image-axiom-mission-pad-39a.html
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission.
Wednesday, 13 April 2022 10:50

Register for Living Planet Symposium 2022

Write a comment

Register for Living Planet Symposium 2022

Write a comment

Press Release N° 16–2022

Following the Russian aggression against Ukraine, ESA’s Director General has initiated a comprehensive review of all activities currently undertaken in cooperation with Russia and Ukraine. The objective is to determine the possible consequences of this new geopolitical context for ESA programmes and activities and to create a more resilient and robust space infrastructure for Europe.

Write a comment
MIRI integration into JWST payload module

With help from a cryocooler, Webb's Mid-Infrared Instrument has dropped down to just a few degrees above the lowest temperature matter can reach and is ready for calibration.

Write a comment
Beijing, China (SPX) Apr 13, 2022
A German team of astronomers from the Universities of Tubingen and Potsdam, led by Prof. Klaus Werner, have discovered a new type of weird stars. The spectra of the star sample, obtained by Large Binocular Telescope in Arizona, USA, and the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) based at Xinglong and operated by the National Astronomical Observatories of the Chi
Page 1344 of 2131