7/ The largest & most important mid-course correction was done 12.5 hours after launch. The #Webb team was at that point able to determine that @ariane5's placement of #Webb was better than requirements #WebbThanksAriane
8/ The team then deployed the gimbaled antenna assembly 📡, which included Webb’s high-data-rate dish antenna. This antenna is used to send at least 28.6 Gbytes of data down from the observatory, twice a day
9/ Part of @esaoperations' #Estrack cooperative network, the 10-m dish in #Malindi, Kenya, was due to make first contact for the all-important 'acquisition of signal’ and so it did.
10/ After a 2nd mid-correction burn, the team determined #Webb should have enough propellant to support science operations in orbit for significantly more than a 10-year lifetime!
12/ Several steps were needed to start deploying #Webb's sunshield 🛡️
✔️ The unfolding of the pallets
✔️ The extension of the observatory’s Deployable Tower Assembly
✔️ Releasing and rolling the sunshield covers
17/ Next were the mirrors. The observatory’s secondary mirror plays an important role in reflecting the light from the primary mirror to where the instruments sit
1/ While we wait for news on L2 orbit insertion, we've got some facts for you on #Webb's orbit 👇
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 🌍 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.
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
📷 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/ 🔴 multi-object spectroscopy mode — #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/ 🔴 fixed slits spectroscopy mode — #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.
📷 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 🌀 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.
🔗 blogs.nasa.gov/webb/2022/01/0…
🎥 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.