Towards the Dawn (12/8/19)
Captain Jeb takes a photo from his seat in the cockpit of a Deuce as they work their way east over the Kerblantic towards the coming day
Above the Storm (12/8/19)
At 6km ASL the crew of the Deuce make ready to dive into the thick of a low-pressure system to capture valuable data about the storm while it is active
Rolling On Out (12/9/19)
The Progeny Mk6 Block I for tomorrow's mission heads for the launch site with the mounting vehicle, tanker truck and crew shuttle following behind. The shadow of the service towers is visible on the VAB doors in front of which is parked the Mobile Launch Platform
Spectators Arrive (12/10/19)
Shuttle buses are seen here leaving the Support Village and carrying visitors over the causeway to KSC so they can view the upcoming launch
Progeny Mk6 Block 1 No.14 (12/10/19)
The third in a series of 4 launches that will carry student-designed and built experiments up into space
Zosimus Pass #4 (12/10/19)
In what turned out to be it's last pass, the debris of the asteroid likely rained down somewhere along this track as it has not been spotted back in orbit in the days since
Mount Kermon (12/11/19)
On the way to the Sheltered Rock region, Captain Jebediah lets the autopilot do its job while he snags a photo of the highest mountain in the KSC region
SRG Afar (12/11/19)
Flying south of Sheltered Rock General airport, seen off in the distance, a passing Deuce is on its way to investigate a storm north of the mountains, hidden over the horizon and behind the tall peaks
Mountain Sunset (12/11/19)
The sun begins to dip behind the mountains of Sheltered Rock as seen from a Deuce belly cam at 6km
Stack It Up (12/12/19)
The final rocket for 2019, a Progeny Mk6 Block I, is being vertically stacked to test load bearing elements. To the rear workers get Ascension Mk1 & Mk2 parts ready to move to "center stage" next year for final assembly
Radiation Study (12/12/19)
The aurora that can be found near the north and south poles are formed from charged particles striking the upper atmosphere after being funneled down along the lines of the magnetic field, which creates a belt of radiation that affects even the surface at high latitudes. This balloon will ascend to 25km to measure these changes in radiation
Radiation Data (12/13/19)
a plot of rad levels collected during the balloon's ascent. The rad increase should be more linear but since the balloon is drifting south towards the edge of where the outer radiation belt meets the atmosphere the increase starts to fall off
