For the first time since 1972, a moon rocket is ready to launch on the first of three sequenced missions to return humanity to the lunar surface. This time to stay.
Liftoff of the Artemis I mission is scheduled for a two-hour launch window that opens at 8:33 AM EDT (12:33 UTC) on Monday, August 29 from LC-39B at the Kennedy Space Center in Florida.
This will be only the second time in history that Pad 39B has hosted a launch to the Moon. The only other flight to do so was the Apollo 10 dress rehearsal for the first lunar landing.
For SLS, the final major configuration of the vehicle will take place with fueling operations that will load 730,000 gallons of liquid hydrogen and liquid oxygen into the Core Stage.
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This major operation will begin with chilldown of the liquid oxygen transfer lines and the propulsion lines in the core stage. If all goes well with the start of liquid oxygen loading, liquid hydrogen fueling will then pick up.
As the Wet Dress Rehearsal campaign showed, the fueling operation is complex and must follow a specific sequence, specifically so that the liquid oxygen Core Stage tank is no more than 50% full by the time liquid hydrogen loading begins. This has to do with the thermal and mass characteristics of the Core Stage.
This process was seen during the Wet Dress Rehearsal campaigns when liquid hydrogen leaks forced a stop to liquid oxygen loading.
The last liquid hydrogen leak during the fourth and final Wet Dress Rehearsal was corrected in the Vehicle Assembly Building through seal replacement and tightening of the connections from the ground side to the vehicle.
Heading into the final part of the count in the overnight hours of August 28 and August 29, the Exploration Ground Systems (EGS) launch team is cautiously optimistic that the liquid hydrogen leaks have been addressed.
During an L-2 day briefing, Artemis I Launch Director Charlie Blackwell-Thompson stated that if all is progressing on the timeline, the liquid hydrogen leak fix should be verified around 3:30 AM EDT (07:30 UTC).
The reason why the teams will not be sure of the fix until this point is that liquid hydrogen leak checks have to be performed with liquid hydrogen. Ambient tests can provide some confidence, as have been performed in the Vehicle Assembly Building, but liquid hydrogen’s low temperature and small molecular size mean only flowing the cryogenic fuel can be the true final test of fix.
If all is proceeding well with Core Stage fuel loading, Interim Cryogenic Propulsion Stage (ICPS) fueling with liquid hydrogen and liquid oxygen will commence thereafter — with the ICPS being the last portion of the vehicle to be fueled for flight.
However, before tanking operations begin, teams need to successfully transition from air purge over to gaseous nitrogen purge. Issues establishing this nitrogen purge during the Wet Dress Rehearsal campaigns resulted in the launch team extending the hold before fueling.
Based on this lesson learned, teams should have more time to work on any issues that arise during the count.
During this period, as propellants are flowing into the vehicle, thermal conditioning of the four RS-25 Core Stage engines will commence. This lengthy process ensures the engines are within the proper “start box” at the end of the countdown.
The “start box” is the range of allowable engine temperatures and pressures that ensure proper ignition and start-up.
The four RS-25 engines on Artemis I are ones that were still in service at the end of the Shuttle program. But, for Artemis I, at least one component on each of the Core Stage engines comes from the three engines that powered Columbia to orbit on STS-1 on April 12, 1981.
“It might be a valve, it might be a bolt, for others, it’s pieces of wiring, little things like that,” said Aerojet Rocketdyne’s Bill Muddle, RS-25 lead field integration engineer, in an interview with NASASpaceflight. “But there is something from the STS-1 engines on each of these [for Artemis I].”
Some changes to the engines for fit and function on SLS have resulted in a slight change to their ignition timing from Shuttle. Instead of igniting at T-6.6 seconds, the four Core Stage RS-25s will begin their ignition sequence at T-6.36 seconds.
Muddle confirmed that the engines will start 120 milliseconds apart from each other for acoustic and vibration considerations just as they did in the Shuttle era.
Ten seconds before engine start, nearly 400,000 gallons of water will begin dumping into the flame trench of LC-39B and the RS-25 and Solid Rocket Booster flame holes in the Mobile Launcher.
Six seconds before engine start, the Hydrogen Burn Off Igniters (HBOIs) will fire across the plane of the RS-25 engine nozzles and upward at the Core Stage Auxiliary Power Unit exhaust ports.
This will ensure that excess hydrogen is safely burned off before the engines start and that any hydrogen is safely burned off should there be an engine shutdown and abort on the pad.
From engine start down to T0, the engines will build up to 100% rated performance thrust within three seconds, after which health checks will confirm the engines are good for the next major event that commits the vehicle to flight: Solid Rocket Booster (SRB) ignition.
At T0, a rapid sequence of events will trigger the swing arms to move away from the vehicle, for the Tail Service Mast fueling and data lines to pull back into their protective doghouse covers, and for the final fire sequence command to be sent to light the SRBs.
The moment the boosters ignite, SLS is committed to lifting off the pad under its own 8.8 million pounds of thrust.
SLS will rise vertically off its Mobile Launcher perched atop LC-39B for seven seconds before the pitch and roll program will maneuver the rocket onto the proper azimuth for its flight to the Moon.
The roll program will initiate at a velocity of 35 meters per second (79 miles per hour).
Max-Q, the moment of maximum stress on the rocket, will be reached at T+ one minute and 10 seconds as the vehicle climbs through 12.9 km (42,500 feet) and accelerates through 447 meters per second (1,000 mph).
SLS on the pad ahead of Artemis I. All seven of my remotes cameras are now set.
Live views: https://t.co/40v5wIEioN pic.twitter.com/zB2AOGzqs8
— Michael Baylor (@nextspaceflight) August 27, 2022
This first stage of flight will see SLS utilize an open loop guidance system, where the rocket follows a pre-programmed pitch profile based on its velocity, altitude, and initial orbital insertion targets.
After constantly changing its pitch as required to reach the desired orbit, an attitude hold will be commanded on the SLS rocket just before the first major event in the launch sequence, SRB separation.
At approximately T+ two minutes and 12 seconds, the twin five-segment SRBs from Northrop Grumman will separate from the Core Stage, having done their job.
This event will be preceded by a lowering of the pressure inside the SRB chamber which will lower the thrust — an event known as “tail off.” This will ensure the boosters have just enough remaining thrust to safely separate.
According to Muddle from Aerojet Rocketdyne, additional thermal coating was needed on small portions of the outside of the engine nozzles of the RS-25s because the SRB separation motors, when fired, will impinge on those locations on the engines.
“Here, [the RS-25s] are literally a couple feet away [from the Solid Rocket Booster separation motors]. So we had to be very careful,” said Muddle.
“The booster separation motors actually point at our engines for about a second, and so working with Northrop Grumman and Boeing, we had to figure out what the heat loads were going to be. And so basically, once you know that, where on the nozzle the heat load is going to be, and how much, then you design more insulation, more ablatives and those types of things.”
At SRB separation, under a nominal mission profile, SLS will be traveling around 1,417 meters per second (3,170 mph) while being 48.1 km (158,000 feet) in altitude.
Approximately one minute later, with the vehicle now flying above the majority of Earth’s atmosphere, the aerodynamic elements protecting Orion can safely be jettisoned.
The three fairing panels surrounding the European Service Module (ESM) will separate at T+ three minutes and 13 seconds, followed by the Launch Abort System (LAS) at T+ three minutes and 19 seconds.
The timing of these events, especially those later in the mission, are approximated based on predicted vehicle performance. The changing trajectory options, based on when in the window that liftoff occurs, can also slightly affect the timing of staging events and burn times.
The core stage will continue to power the ascent for several more minutes, targeting an unstable 30 x 1805 km orbit. The 30 km perigee, while above the Earth’s surface, is well within the atmosphere. This trajectory ensures that the Core Stage safely reenters during its first orbit, breaking apart over a designated area of the Pacific Ocean. The 1805 km apogee gives the combined ICPS and Orion stack enough energy to, with two burns, reach the Moon.
After Main Engine Cutoff (MECO) at T+ eight minutes and four seconds, the ICPS and Orion stack will separate from the core stage at T+ eight minutes and 16 seconds. For ICPS and Orion to avoid the same fate as the core stage, the stack will coast up to apogee before performing the first of two ICPS burns. This perigee raise burn will increase the perigee to over 800 km.
During this coast phase, Orion’s four solar arrays will deploy, beginning about 18 minutes and 20 seconds after liftoff. Solar array deployment takes approximately 12 minutes.
The ICPS, itself a slightly modified Delta Cryogenic Second Stage (DCSS) from United Launch Alliance’s Delta IV rocket family, is powered by a single RL-10-B-2 engine. According to Aerojet Rocketdyne’s Nicole Cummings, RL-10 & Exploartion Upper Stage Deputy Program Manager, in an interview with NASASpaceflight, this will be the final RL-10-B-2 engine to fly.
“The ICPS, it is historic to watch it fly our last B-2,” said Cummings. But engine upgrades to the RL-10-C line for better performance are planing and integrated for the ICPS components for Artemis II and III before the RL-10-C-3 engines take over on the Exploration Upper Stage for Artemis IV and beyond.
The RL-10-B-2 for Artemis I will begin the perigee raise burn at T+ 51 minutes and 22 seconds, and the engine will shut down 22 seconds later.
Following another coast phase for ICPS and Orion until perigee, the Trans-Lunar Injection (TLI) burn will occur. This maneuver raises the orbital apogee out to the Moon, allowing Orion to later insert itself into the desired Distant Retrograde Orbit. This second ICPS burn begins at T+ one hour and 37 minutes and lasts approximately 18 minutes.
Orion will separate from ICPS at T+ two hours, six minutes, and 10 seconds. Shortly after, and T+ two hours, seven minutes, and 31 seconds, Orion’s thrusters will fire briefly to distance the spacecraft from ICPS.
With Orion delivered to its Trans-Lunar trajectory, ICPS conducts one final burn at T+ three and a half hours to safely dispose of itself into a heliocentric orbit.
Orion’s next maneuver will not occur until almost six hours later when the service module’s main engine ignites for a planned Outbound Trajectory Correction-1 burn. After a nominal liftoff, ascent, and a handful of on-orbit maneuvers, Orion will coast for a few days before Artemis I action picks right back up at the moon on flight day six.
(Lead image: SLS on the pad ready for launch. Credit: Thomas Burghardt for NSF)
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