1/ While we wait for news on L2 orbit insertion, we've got some facts for you on #Webb's orbit π
2/ Unlike @Hubble_Space#Webb will not be in orbit around the Earth, but will orbit the Sun, 1.5 million km away from the π at what is called the second Lagrange point or L2.
3/ This orbit lets the telescope stay in line with the Earth as it moves around the Sun. This allows the satellite's large sunshield to protect the telescope from the light and heat of the Sun, Earth and Moon.
4/ Webb's sunshield gives the telescope the equivalent of SPF one million sunscreenπ§΄! For that to be effective protection against the light and heat of the Sun/Earth/Moon, these bodies all have to be located in the same direction. This is what L2 provides.
5/ There are actually 5 Lagrange points, that is, a configuration in which three bodies could orbit each other, yet stay in the same position relative to each other
6/ L1 is 1.5 million km from the Earth towards the Sun, and there have been many solar observatories located there, including DSCOVR, WIND, @MissionSoho & ACE.
8/ L4 and L5 are stable in that objects there will orbit L4 and L5 with no assistance. Some small asteroids πͺ¨ are known to be orbiting the Sun-Earth L4 and L5 points.
9/ L1, L2, and L3 are metastable so objects around these points slowly drift away into their own orbits around the Sun unless they maintain their positions, for example by using small periodic rocket thrust. This is why L1, L2, and L3 don't "collect" objects like L4 and L5 do.
10/ At L2, #Webb is orbiting the Sun further out than Earth, so how long does it take Webb to make a full orbit around the Sun?
11/ Webb will not sit stationary precisely at L2, but orbit around L2. This orbit keeps the telescope out of the shadows of both the Earth and Moon. Unlike @HUBBLE_space, which goes in and out of Earth shadow every 90 minutes, #Webb will have science operations 24/7.
12/ Webb's orbit around L2 is actually similar in size to the Moon's orbit around the Earth! But how long does it take #Webb to orbit L2?
13/ #Webb's position at L2 makes comms easier π. Since it will always be at the same location relative to Earth we can have continuous communications with it as the π rotates through the Deep Space Network, using 3 large π‘ located in Australia, Spain & US (California)
1/ The Mid-InfraRed Instrument #MIRI is one of 4 instruments on the James #Webb Space Telescope. The only mid-infrared instrument in its instrument suite. #WebbSeesFarther
π· NASA/ Chris Gunn
2/ Thanks to state-of-the-art instrument design and components, it will deliver mid-infrared images and spectra with an unprecedented combination of sharpness and sensitivity. #WebbSeesFarther
3/ #MIRI will be capable of penetrating thick layers of dust obscuring regions of intense star birth. It will see the first generations of galaxies to form after the #BigBang, and it will study sites of new planet formation and the composition of the interstellar medium.
1/ #NIRSpec has three modes of operation: multi-object spectroscopy mode, fixed slits spectroscopy mode and integral field spectroscopy mode:
2/ π΄ multi-object spectroscopy mode β #NIRSpec will be the 1st multi-object spectrograph in space, able to record the spectra of up to 200 objects at the same time. A capability enabled by microshutters.
3/ π΄ fixed slits spectroscopy mode β #NIRSpec will also be able to carry out single-object, high-contrast spectroscopy using a set of five fixed slits. It will provide high contrast spectra of sources and a key to the study of exoplanets.
1/ As we wait for full mirror deployment, here are some cool-to-know facts about #Webb 's mirrors.
π· Northrop Grumman, NASA/Chris Gunn
2/ #Webb has a primary mirror 6.5m across as this is what was needed to measure the light from very young galaxies π over 13 billion light years away.
3/ A mirror this large had never before been launched into space! If the @HUBBLE_space 2.4 m glass mirror were scaled to be large enough for #Webb, it would be too heavy to launch into orbit.
1/ While everyone's eyes were on the shield tensioning, the Mid-Infrared Instrument (MIRI) provided by @esa for #Webb also had an important milestone: unlocking the Contamination Control Cover, which had to be locked for launch.
π blogs.nasa.gov/webb/2022/01/0β¦
π₯ ESA/ATG medialab
@esa 2/ After successfully completing the tests and unlocking the cover, the instrument control electronics were then powered off before the next steps on the sunshield tensioning activities.
@esa 3/ This key step for MIRI was monitored remotely by team members in Europe, ready to provide assistance if it were needed.