Behind the Scenes of the Final Frontier: Our Tour with NASA’s “Launch Director” – 1

Discover an insider’s voyage to the heart of NASA’s launch operations with us as we relive the awe-inspiring Kennedy Space Center Tour, where every corner whispers tales of cosmic ventures and human courage.

Introduction

Late winter 2017 my wife Pam and I embarked on an extraordinary adventure that would etch an indelible mark on our memories. On March 2nd, we had the unique privilege of experiencing the Kennedy Space Center through the eyes of a NASA Launch Director. This wasn’t just any tour; it was a journey through the heart of space exploration, a narrative brought to life by someone who had been at the helm of launching dreams into the cosmos.

The Kennedy Space Center, a beacon of human achievement on Florida’s coastline, stood before us, brimming with stories of courage, innovation, and the relentless pursuit of the unknown. As we stepped onto the grounds, we were not just visitors but participants in a legacy stretching back to the earliest days of space travel. The “NASA Launch Director Tour” promised an inside look at the complexities and triumphs of space missions, a perspective few ever witness.

This series of blog posts is an attempt to capture the essence of that day, to share the insights, emotions, and awe-inspiring moments we experienced. From the thunderous silence of the launch pads to the intimate stories of missions past, each post will explore a different facet of our journey. Join us as we relive an unforgettable exploration of human ingenuity and the boundless reaches of space, all through the lens of a day that brought the stars within reach.

Gathering and Introductions

On the negative side, we enjoyed the expertise of “Jeff” who stood in for the retired Launch Director who was “out sick.” On the positive side, our very expensive fee for the tour was refunded. Jeff was everything we could expect from the tour — he had extensive and detailed insider knowledge of NASA and the launch facilities.

Jeff, our substitute guide

We gathered in a media room, an antechamber to the Space Shuttle Atlantis.

Entry to the Atlantis and the

Space Shuttle Atlantis lifted off on its maiden voyage STS-51-J on October 3, 1985. This was the second shuttle mission that was a dedicated Department of Defense mission. It flew one other mission, STS-61-B (the second shuttle night launch) before the Challenger disaster temporarily grounded the shuttle fleet in 1986. Among the five Space Shuttles flown into space, Atlantis conducted a subsequent mission in the shortest time after the previous mission (turnaround time) when it launched in November 1985 on STS-61-B, only 50 days after its previous mission, STS-51-J in October 1985. Atlantis was then used for ten flights from 1988 to 1992. Two of these, both flown in 1989, deployed the planetary probes Magellan to Venus (on STS-30) and Galileo to Jupiter (on STS-34). With STS-30 Atlantis became the first Space Shuttle to launch an interplanetary probe.

The orbiter’s aluminum structure could not withstand temperatures over 175 °C (347 °F) without structural failure. Aerodynamic heating during reentry would push the temperature well above this level in areas, so an effective insulator was needed.

The Thermal protection system (TPS) covered essentially the entire orbiter surface, and consisted of seven different materials in varying locations based on amount of required heat protection:

–Reinforced carbon–carbon (RCC), used in the nose cap, the chin area between the nose cap and nose landing gear doors, the arrowhead aft of the nose landing gear door, and the wing leading edges. Used where reentry temperature exceeded 1,260 °C (2,300 °F).

Reinforced carbon–carbon (RCC) of the nose cap and “chin area”


–High-temperature reusable surface insulation (HRSI) tiles, used on the orbiter underside. Made of coated LI-900 silica ceramics. Used where reentry temperature was below 1,260 °C.
–Fibrous refractory composite insulation (FRCI) tiles, used to provide improved strength, durability, resistance to coating cracking and weight reduction. Some HRSI tiles were replaced by this type.
–Flexible Insulation Blankets (FIB), a quilted, flexible blanket-like surface insulation. Used where reentry temperature was below 649 °C (1,200 °F).

–Low-temperature Reusable Surface Insulation (LRSI) tiles, formerly used on the upper fuselage, but were mostly replaced by FIB. Used in temperature ranges roughly similar to FIB.
–Toughened unipiece fibrous insulation (TUFI) tiles, a stronger, tougher tile which came into use in 1996. Used in high and low temperature areas.
–Felt reusable surface insulation (FRSI). White Nomex felt blankets on the upper payload bay doors, portions of the mid fuselage and aft fuselage sides, portions of the upper wing surface and a portion of the OMS/RCS pods. Used where temperatures stayed below 371 °C (700 °F).
Each type of TPS had specific heat protection, impact resistance, and weight characteristics, which determined the locations where it was used and the amount used.

The shuttle TPS had three key characteristics that distinguished it from the TPS used on previous spacecraft:

Reusable
Previous spacecraft generally used ablative heat shields which burned off during reentry and so could not be reused. This insulation was robust and reliable, and the single-use nature was appropriate for a single-use vehicle. By contrast, the reusable shuttle required a reusable thermal protection system.
Lightweight
Previous ablative heat shields were very heavy. For example, the ablative heat shield on the Apollo Command Module comprised about 15% of the vehicle weight. The winged shuttle had much more surface area than previous spacecraft, so a lightweight TPS was crucial.
Fragile
The only known technology in the early 1970s with the required thermal and weight characteristics was also so fragile, due to the very low density, that one could easily crush a TPS tile by hand.

Reinforced carbon–carbon (RCC) of the nose cap, close-up

The Space Shuttle thermal protection system (TPS) is the barrier that protected the Space Shuttle Orbiter during the searing 1,650 °C (3,000 °F) heat of atmospheric reentry. A secondary goal was to protect from the heat and cold of space while in orbit.


During the launch of STS-27 in 1988, a piece of insulation shed from the right solid rocket booster struck the underside of the vehicle, severely damaging over 700 tiles and removing one tile altogether. The crew were instructed to use the remote manipulator system to survey the condition of the underside of the right wing, ultimately finding substantial tile damage. Due to the classified nature of the mission, the only images transferred to the mission control center were encrypted and of extremely poor quality. Mission control personnel deemed the damage to be “lights and shadows” and instructed the crew to proceed with the mission as usual, infuriating many of the crew. Upon landing, Atlantis became the single-most-damaged shuttle to successfully land. The survival of the crew is attributed to a steel L band antenna plate which was positioned directly under the missing tile. A similar situation would eventually lead to the loss of the shuttle Columbia in 2003, albeit on the more critical reinforced carbon-carbon.

References: extensive sections of the following Wikipedia articles were quoted, "Space Shuttle thermal protection system," "Space Shuttle  Atlantis."

Copyright 2024 Michael Stephen Wills All Rights Reserved

Thin Crescent with McGraw Tower, Venus and Star

Here I revel in the spectacle of an early morning rising of the cresent moon.

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Thin Crescent Bowl filled with Earthglow

Here I explore the concepts of “earthglow” and occultation.

Continue reading “Thin Crescent Bowl filled with Earthglow”

Venus at dawn

Planet Thoughts

Since 1500 B.C. until today…..

The planet we call Venus has ancient associations with fertility goddesses. The link has persisted at least from the 1600 century B.C. inscribed on Sumerian cuneiform tablets. Three thousand years later the Italian artist Botticelli created in tempura paint on canvas the image of Venus rising from the sea, as the planet Venus does today.

Venus Rising

Here is Venus rising from the sea at dawn January 2022, at its brightest and most beautiful. Some mistake this new light in the east for airplane lights; the bright disk of Venus is 25 times brighter than Sirius, enough to cast shadows at night. As Venus proceeds in its orbit, the planet alternately sets after the sun and rises before it, seemingly appearing new each time.

This February I caught a newly risen Venus in this IPhone 7 video, reflected in the waves. It seemed to be a flashing headlight on the beach, the Venus reflection came and went with the passing waves. Venus is the upper, the reflection is beneath. Use the lower right control for the full view.

Looking from his window June 1889, Vincent VanGogh included Venus in his “Starry Night” painting, seen to the right of the Cypress tree.

Here is a closer view of Venus last January, the planet disk is apparent, unlike even the closest stars, Venus is seen as a whole object. Click on image for a full view.

Venus and Mars

Venus and Mars shared 2022’s pre-dawn winter sky. Click on the first image for a full-size view. Mars is seen above the palm tree stump, on the right. In this photograph, from early February, Venus and Mar apparently moved closer. The closeness is an illusion, the planets are millions of miles apart, on either side of Earth’s orbit. Click on the photograph for a full-size view, Mars can just be made out to the right and above Venus.

This crop clearly shows the brightness of Venus compared to Mars.

Thin Crescent with McGraw Tower, Venus and Star

pre-dawn sky event

Here are two photographs taken about the same time, 6:30 am, October 18, 2017, companions to the photograph shared earlier this week.

The moon rises later each day, so these shots include a larger disk closer to Cornell University.  Both components, the crescent and earth-glow, were dimmer this morning.    In each photograph Jenny McGraw Tower is visible.

Crescent, McjGraw Tower, Regulus, Venus
The star is Regulus, the brightest in the constellation Leo, close below the moon.  I don’t know the star close to Venus.

Here the tower is slightly to the right of the crescent, the arch of Schoellkopf stadium further right.  Among the trees on left, is the baleful red glow of Bradford Hall.

Cresent, McGraw Tower, Regulus
Click for another view of McGraw Tower from my Online gallery.

The tower is outlined by the lights of Uris library, presumably filled with early rising students.

The light of Regulus (“small king”),  below and to the right, is a composite of four stars moving together through space.  The position of Regulus on the path in the sky of the moon, planets and asteroids (called the ecliptic) leads to the occultation of the star by the disks of the moon and, less regularly, the planets and asteroids.

Copyright 2021 Michael Stephen Wills All Rights Reserved

Thin Crescent Bowl filled with Earthglow

pre-dawn sky event

A thin crescent bowl filled with earthglow floating above the dawn attended by Venus, Mars, Virgo.

Thin Crescent with Planets, Stars, Dawn

This was the view from Ithaca, New York at the start of dawn this morning of Tuesday, October 17, 2017.  Mars is next to the moon, the stars of the constellation Virgo scattered around, Venus is the bright object below.  We had a bright, clear sky not unusual for September and October.

Want more? Click the link for my Online Gallery

In the city, an arch of Schoellkopf Stadium on the Cornell University campus.  Cornell is on east hill.  We live on west hill, across the valley.  It is quiet on west hill, away from the students.

Earlier this week the crescent was in the constellation Leo where the bright limb occulted the bright star Regulus, to reappeared from behind the dark limb, a brilliant spectacle that happened after dawn for New York.  It was cloudy, as usual, on October 14.

When I woke, the moon was shining through the trees, still full of just turning leaves. The crescent turned, cup like, above the horizon, to cradle the dark orb glowing from the reflected light of our earth. I did not recognize Mars, the disk was less red than usual. Research revealed the moon had two planets in seeming attendance. I also learned that, when the horns point right the moon is waning, moving toward a new, or un-illuminated, moon. When the phase moved from new it is also a crescent with horns pointing left.

This morning was a fortunate gift, I had never contemplated the moon in quite this form before.

Copyright 2021 Michael Stephen Wills All Rights Reserved

International Space Station

pre-dawn sky event

December 23rd, sky clear at 6:30 am, the International Space Station (ISS) passed through the zenith with a waning crescent, a bowl filled with earthglow, in the southeast. On December 22nd I received the following email from NASA advising me of the event.

HQ-spotthestation@mail.nasa.gov

Sun 12/22/2019 7:00 PM

Time: Mon Dec 23 6:30 AM, Visible: 6 min, Max Height: 87°, Appears: 10° above SW, Disappears: 11° above ENE

Visit the NASA site to research if ISS viewing is possible from your location.

Here is another photograph of the crescent moon filled with earthglow.

Click photograph for the expanded view. To do this from WordPress Reader, you need to first click the title of this post to open a new page.
Copyright 2020 All Rights Reserved Michael Stephen Wills

Earthglow

pre-dawn sky event

December 23rd, sky clear at 6:30 am, the International Space Station passed through the zenith with a waning crescent, a bowl filled with earthglow, in the southeast. Here is a photograph of a waning moon above Cornell University from October 2017.

Copyright 2024 All Rights Reserved Michael Stephen Wills