Let’s take a look at JWST mirrors.
Besides the familiar large primary mirror, JWST contains 3 other mirrors – a secondary mirror mounted at the end of the tripod struct, a tertiary mirror and a fine steering mirror. The figure below shows the path of IR light across the mirrors.
We all know that the JWST primary mirror is composed of 18 hexagonal mirror segments.
Each mirror segment is 1.3 meters from side-to-side, 2 inches thick and weighs 40 kg.
The mirror is made of Beryllium, atomic number = 4, a stiff and light-weight metal, 4.2 times lighter than steel, a good conductor of electricity and heat and excellent at holding its shape across a wide range of temperatures.
The flat surface of each mirror has been precisely ground, polished and coated with a thin layer of gold; gold improves the mirror's infrared light reflectivity. A thin layer of amorphous SiO2 (glass) is deposited on top of the gold to protect it from scratches during handling.
The following video shows the mirror's odyssey across the US. Fabrication steps include Beryllium ore mining and purification, pressing of Be and cutting of mirror blanks, shaping and polishing of mirrors, gold plating and cryogenic cooling and testing.
Each mirror can be independently shifted, tilted and bent using a set of actuators to achieve precise focus across all 18 segments.
The back of the Be mirror is milled out to reduce weight, leaving a honeycomb structure of ribs that provides stiffness and support to the mirror.
A number of structures, many made with Beryllium, are mounted behind each mirror, including 7 actuators. Six (degrees of freedom (DOF)) actuators enable each mirror to be very precisely shifted and tilted to optimal position.
The 7th radius-of-curvature (RoC) actuator and set of 6 struts enable the mirror surface to be bent and curved. The mirrors will be precisely aligned and curved after they reach their operational temperature in L2 orbit. They will fine-tuned every 2 weeks thereafter.
The secondary mirror is a circular convex shaped mirror, 0.74 meters in diameter, made of gold-plated Beryllium. The curvature of the mirror was created during fabrication and polishing. It is mounted at the end of the tripod-like secondary mirror support structure (SMSS).
Here is a comparison of optical telescope primary mirror sizes. JWST and Hubble are at the bottom left.
JWST’s 6.5m mirror is 6.25 times large than Hubble’s 2.4m mirror, in light collecting area.
Source: commons.wikimedia.org...
Please take a look at this thread for how #JWST is pointed at its target of interest.
The GSE Handling Ring in the above JWST mirror pic is part of a test fixture and not used in flight.
The pic also clearly shows the machined out back side of the mirror with the egg-crate-like mesh structure providing support to the mirror.
Source: spiedigitallibrary.org/journals/optic…
The JWST actuators use stepper motors plus gears, couplers and cams to produce linear motion with sub-10 nm accuracy.
See authors.library.caltech.edu/91580/1/106983… for more details.
FYI - The JWST secondary mirror also uses actuators for positioning and tilting. I don't think it uses an actuator for curvature control.
Some additional info from spacesymposium.org/wp-content/upl… - the JWST primary mirror segments are curved during fabrication, but not to a very low tolerance. The RoC actuators will be used for precise modification of the mirror surface curvature during the next few months.
Here is some more data on #JWST mirrors and their placement on the spacecraft. E.g., the secondary mirror is 7.169 meters away from the primary mirror. The tertiary and fine steering mirrors are slightly offset from the boresight line. EFL is the effective focal length.
Here are pics of the #JWST tertiary and fine steering mirrors. Note that the tertiary mirror has a rectangle-like shape 0.728 m x 0.517 m. The fine steering meter is 0.172 m in diameter and has a similar shape as the primary mirror.
Let's take a look at the unfolding and latching of the #JWST mirror wings yesterday. Each wing has 2 hinges, similar to door hinges. One of the hinges was driven by a motor, which rotated the wing into its position aligned with the main mirror assembly.
The inner edge of the wing has 4 sets of latches. Each latch set contains 2 guide latches and one middle latch with a nut. The edge of the main mirror assembly has corresponding guide latches and the middle latches each with a screw. The screw is driven by a stepper gear motor.
The screws were engaged once the wing was almost fully opened. It took a few hours yesterday to methodically align and fasten the latches and to achieve precise alignment of the wing mirrors with the main assembly.
See esmats.eu/amspapers/past… for more details.
Around May 24, JWST sustained a dust-sized micrometeroid impact to its primary mirror segment C3. Initial assessment shows that the telescope's performance remains above all mission requirements although there is a marginally detectable effect in its data. 1/
The size of the micrometeroid and the physical nature of the damage are not clear from the report. JWST does not have cameras to observe such damage. The impact of the micrometeroid is judged based on its effect on image quality.
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Such micrometeroid events are expected and have been simulated and tested on the ground. Since launch, there have been 4 smaller measurable micrometeoroid strikes; the latest one is larger than the degradation predictions assumed by JWST engineers. 3/
While #MarsHelicopter Ingenuity is learning how to fly with a broken Inclinometer, Mars Rover Perseverance has been been busy roaming the "bacon strip" area near the Delta region, looking for interesting rocks. Hopefully, it will find one worthy of a rock core collection soon. 1/
This is the current location of Perseverance, right on top of the "bacon strip". Percy is probably hesitant to climb up the delta until Ingenuity moves to a better location, since Ingenuity needs Percy to communicate with earth. 2/
The approach to the "bacon strip" area on June 6 - 3/
Update on #MarsHelicopter Ingenuity. As the heaters and electronics have been shut off at night to conserve power, one of the navigation sensors, called the inclinometer, has stopped functioning. But the team will still be able to fly it soon using some spare accelerometers. 1/
The inclinometer's two accelerometers measure gravity prior to spin-up and takeoff; the direction of the sensed gravity is used to determine Ingenuity's orientation. NASA scientists had created a backup method to generate this data before Perseverance landed on Mars!
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The Inertial Measurement Unit (IMU) contains accelerometers which can provide similar but less accurate data. The new software, already being uploaded, will in real-time patch this data in place of the data from the Inclinometer.
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The Artemis @NASA_SLS rocket left the Vehicle Assembly Building around 12:01am ET earlier today and completed its four-mile trek to Launch Complex 39B around 8:20 a.m. EDT.
Let’s take a look at the unique NASA crawler-transporter vehicle used for this purpose. 1/
A pair of crawlers (nicknamed “Hans” and “Franz”) were built in 1965 to move the massive Saturn V rocket from Kennedy’s Vehicle Assembly Building to Launch Complex 39. After the Moon landing and Skylab programs ended, the crawlers were used to transport the space shuttles. 2/
CT-2 was upgraded for the Artemis program around 2012 with new generators, control system modifications, diesel engine refurbishments and upgraded roller bearings.
CT-1 was originally planned for commercial launch vehicles but its future remains uncertain. 3/
Where is Mars Rover Perseverance and where is it headed next?
The map below shows its path over the past few days, as it traveled west and then doubled back.
Mars Helicopter Ingenuity is parked about 1 km east after its Flight 28 on Apr 29. 1/
It appears that Perseverance is going to try the alternate route through an area called Hawksbill Gap to climb up the Jezero crater delta region. The diagram below includes some guesses for the new route. 2/
During its journey through the region called the Enchanted Lake, no samples were collected in anticipation of more geologically interesting rocks along Perseverance's long journey. mars.nasa.gov/mars2020/missi…
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The Boeing Orbital Flight Test-2 #Starliner began its journey to @ulalaunch's Space Launch Complex-41. By the end of the day, Starliner wil be mated to the #AtlasV rocket. Launch is scheduled for May 19.
But it had a rather jarring glitch on the way 🙁