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55 Years Ago: Six Months Until the Moon Landing

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The new year of 1969 dawned with optimism that NASA would meet President John F. Kennedy’s goal of landing a man on the Moon and returning him safely to the Earth. The previous year saw four Apollo missions, two uncrewed and two carrying three astronauts each, test different components of the lunar landing architecture, culminating with Apollo 8’s December flight around the Moon. Challenges remaining for the new year included testing the Lunar Module (LM) with a crew, first in Earth orbit, and then in lunar orbit, a flight that served as a dress rehearsal for the Moon landing that could take place on the following mission. With flights occurring every two months, engineers at NASA’s Kennedy Space Center (KSC) in Florida processed three spacecraft and launch vehicles in parallel.

Recovering from the fire

The Apollo 1 crew of Virgil I. “Gus” Grissom, left, Edward H. White, and Roger B. Chaffee Liftoff of the first Saturn V on the Apollo 4 mission The Lunar Module for the Apollo 5 mission Recovery of the Apollo 6 Command Module
Left: The Apollo 1 crew of Virgil I. “Gus” Grissom, left, Edward H. White, and Roger B. Chaffee. Middle left: Liftoff of the first Saturn V on the Apollo 4 mission. Middle right: The Lunar Module for the Apollo 5 mission. Right: Recovery of the Apollo 6 Command Module.

The years 1967 and 1968 proved turbulent for the world. For NASA, the focus remained on recovering from the tragic Apollo 1 fire in time to meet President Kennedy’s fast approaching end of the decade deadline. The fire resulted in a thorough redesign of the Command Module (CM) to reduce flammability risks and to include an easy to open hatch. Engineers also removed flammable materials from the Lunar Module (LM). In November 1967, the first flight of the Saturn V carried Apollo 4 on a nine-hour uncrewed mission to test the CM’s heat shield. Apollo 5 in January 1968 completed an uncrewed test of the LM so successful that NASA decided to cancel a second test. Although fraught with problems, the April 1968 flight of Apollo 6 tested the CM heat shield once again. Managers believed that engineers could solve the problems encountered during this mission and declared that the next Saturn V would carry a crew.

Apollo 7 and 8

Apollo 7 astronauts Walter M. Schirra, left, Donn F. Eisele, and R. Walter Cunningham on the recovery ship USS Essex following their 11-day mission The famous Earthrise photograph from Apollo 8
Left: Apollo 7 astronauts Walter M. Schirra, left, Donn F. Eisele, and R. Walter Cunningham on the recovery ship USS Essex following their 11-day mission. Right: The famous Earthrise photograph from Apollo 8.

By October 1968, thorough ground testing of the Apollo spacecraft enabled the first crewed mission since the fire. Apollo 7 astronauts Walter M. Schirra, Donn F. Eisele, and R. Walter Cunningham successfully completed the 11-day test flight, achieving all mission objectives. In August, with LM development running behind schedule, senior NASA managers began discussions of sending Apollo 8 on a circumlunar flight, pending the outcome of Apollo 7. With that hurdle successfully cleared, astronauts Frank Borman, James A. Lovell, and William A. Anders orbited the Moon 10 times during Christmas 1968, taking a giant leap toward achieving the Moon landing.

At the White House, Apollo 8 astronauts Frank Borman, James A. Lovell, and William A. Anders present a copy of the Earthrise photograph to President Lyndon B. Johnson Accompanied by Vice President Hubert H. Humphrey, Borman, Lovell, and Anders take a motorcade from the White House to the Capitol Borman, left, Lovell, and Anders address a joint meeting of Congress
Left: At the White House, Apollo 8 astronauts Frank Borman, James A. Lovell, and William A. Anders present a copy of the Earthrise photograph to President Lyndon B. Johnson. Middle: Accompanied by Vice President Hubert H. Humphrey, Borman, Lovell, and Anders take a motorcade from the White House to the Capitol. Right: Borman, left, Lovell, and Anders address a joint meeting of Congress.

With their space missions completed, the Apollo 7 and 8 crews remained busy with events celebrating their successes. On Jan. 3, 1969, TIME magazine named Apollo 8 astronauts Borman, Lovell, and Anders their Men of the Year for 1968. Kicking off a whirlwind of events, on Jan. 9, outgoing President Lyndon B. Johnson welcomed them to the White House, where he presented them with NASA Distinguished Service Medals. They in turn presented him with a copy of the famous Earthrise photograph. Accompanied by Vice President Hubert H. Humphrey, Borman, Lovell, and Anders rode in a motorcade down Pennsylvania Avenue to the Capitol where the astronauts addressed a joint meeting of Congress. From there, they proceeded to the State Department for a press conference, their day ending with a dinner in their honor at the Smithsonian Institution.

Apollo 8 astronauts James A. Lovell, left, Frank Borman, and William A. Anders wave to the crowds assembled along their parade route in New York City Borman, Lovell, and Anders address a crowd at Newark airport In Miami’s Orange Bowl Lovell, left, Borman, and Anders lead the fans in the Pledge of Allegiance at Super Bowl III
Left: Apollo 8 astronauts James A. Lovell, left, Frank Borman, and William A. Anders wave to the crowds assembled along their parade route in New York City. Middle: Borman, Lovell, and Anders address a crowd at Newark airport. Right: In Miami’s Orange Bowl Lovell, left, Borman, and Anders lead the fans in the Pledge of Allegiance at Super Bowl III.

On Jan. 10, New York City held a tickertape parade for Borman, Lovell, and Anders. Mayor John V. Lindsay presented them with Medals of the City of New York, after which they attended a luncheon at Lincoln Center, a reception at the United Nations, and dinner at the Waldorf-Astoria Hotel. The next day, in 15-degree weather, they spoke to a crowd of about 1,500 people at Newark Airport before boarding a plane for much warmer Miami, where on Jan. 12 they attended Super Bowl III, and led the Orange Bowl crowd in reciting the Pledge of Allegiance.

In Houston, Apollo 8 astronauts William A. Anders, left, Frank Borman, and James A. Lovell present an Earthrise photograph and flags of Texas to Governor John B. Connally, far right, and Mayor Louie Welch, hidden behind the photograph Borman and his family in the parade through downtown Houston, with Lovell and Anders and their families following behind Lovell, Borman, and Anders wave to the crowds in the parade in Chicago
Left: In Houston, Apollo 8 astronauts William A. Anders, left, Frank Borman, and James A. Lovell present an Earthrise photograph and flags of Texas to Governor John B. Connally, far right, and Mayor Louie Welch, hidden behind the photograph. Middle: Borman and his family in the parade through downtown Houston, with Lovell and Anders and their families following behind. Right: Lovell, Borman, and Anders wave to the crowds in the parade in Chicago.

A crowd estimated at about 250,000 welcomed Borman, Lovell, and Anders home to Houston on Jan. 13. In a ceremony outside the Albert Thomas Convention Center, Mayor Louie Welch presented them with bronze medals for heroism, and the astronauts presented Welch and Texas Governor John B. Connally with plaques bearing Texas flags they had flown to the Moon as well as a framed copy of the Earthrise photograph. The astronauts took part in the largest parade in the city’s history. The next day, the city of Chicago welcomed Borman, Lovell, and Anders. An estimated 1.5 million people cheered them on their parade route to a reception where they received honors from city council.

The Apollo 7 Command Module and a Lunar Module mockup on a float in President Richard M. Nixon’s inauguration parade; Apollo 7 astronauts Walter M. Schirra, R. Walter Cunningham, and Donn F. Eisele preceded the float in an open-air limousine Apollo 8 astronauts Frank Borman, left, James A. Lovell, and William A. Anders with President Nixon at the White House
Left: The Apollo 7 Command Module and a Lunar Module mockup on a float in President Richard M. Nixon’s inauguration parade; Apollo 7 astronauts Walter M. Schirra, R. Walter Cunningham, and Donn F. Eisele preceded the float in an open-air limousine. Image credit: courtesy Richard Nixon Library. Right: Apollo 8 astronauts Frank Borman, left, James A. Lovell, and William A. Anders with President Nixon at the White House.

On Jan. 20, Apollo 7 astronauts Schirra, Eisele, and Cunningham rode in President Richard M. Nixon’s inauguration parade in Washington, D.C. Their spacecraft and a LM mockup rode on a float behind them. Ten days later, the new President invited Apollo 8 astronauts Borman, Lovell, and Anders to the White House where he announced that Borman and his family would embark on an 18-day goodwill tour of eight European nations, starting on Feb. 2.

Apollo 9

The LM remained the one component of the lunar landing architecture not yet tested by astronauts in space. That task fell to James A. McDivitt, David R. Scott, and Russell L. Schweickart, the crew of Apollo 9. They and their backups Charles “Pete” Conrad, Richard F. Gordon, and Alan L. Bean spent many hours in the LM simulators and training for the spacewalk component of the mission.

In preparation for the Apollo 9 spacewalk, astronaut Russell L. Schweickart tests the Portable Life Support System backpack in an altitude chamber at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston Schweickart trains for his spacewalk in MSC’s Water Immersion Facility Apollo 9 backup astronauts Richard F. Gordon, left, and Alan L. Bean train for the spacewalk in the KC-135 zero-gravity aircraft
Left: In preparation for the Apollo 9 spacewalk, astronaut Russell L. Schweickart tests the Portable Life Support System backpack in an altitude chamber at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston. Middle: Schweickart trains for his spacewalk in MSC’s Water Immersion Facility. Right: Apollo 9 backup astronauts Richard F. Gordon, left, and Alan L. Bean train for the spacewalk in the KC-135 zero-gravity aircraft.

Apollo 9’s 10-day mission would take place in the relative safety of low Earth orbit. After docking with the LM, the crew’s first major task involved the first spacewalk of the Apollo program and the only in-space test of the new A7L spacesuit before the Moon landing. McDivitt and Schweickart planned to enter the LM, leaving Scott in the CM. Schweickart and Scott would each perform a spacewalk from their respective spacecraft. Scott would only stand in the open CM hatch while Schweickart would exit via the LM’s front hatch onto its porch, translate over to the CM using handrails, retrieve materials samples mounted on the spacecraft’s exterior and return back to the LM, spending two hours outside. This spacewalk tested the ability of crews to transfer through open space, in case a malfunction with the tunnel or hatches between the two spacecraft prevented an internal transfer. The day after the spacewalk, McDivitt and Schweickart planned to undock the LM, leaving Scott in the CM, fly it up to 100 miles away, testing its descent and ascent stages before returning to Scott in the CM who would perform the rendezvous and docking.

Apollo 9 rollout from the Vehicle Assembly Building to Launch Pad 39A at NASA’s Kennedy Space Center in Florida Apollo 9 rollout from the Vehicle Assembly Building to Launch Pad 39A at NASA’s Kennedy Space Center in Florida Apollo 9 rollout from the Vehicle Assembly Building to Launch Pad 39A at NASA’s Kennedy Space Center in Florida
At NASA’s Kennedy Space Center in Florida, three views of the Apollo 9 rollout from the Vehicle Assembly Building to Launch Pad 39A.

The first of the three vehicles in processing flow at KSC, Apollo 9 rolled out from High Bay 3 of the Vehicle Assembly Building (VAB) to Launch Pad 39A on Jan. 3, just 13 days after Apollo 8 launched from the same facility, causing relatively minor damage. Stages of the Apollo 9 Saturn V had arrived at KSC during the spring and summer of 1968, the LM arrived in June and the Command and Service Modules (CSM) in October. Workers completed stacking of the Saturn V in October, adding the Apollo spacecraft in early December. On Jan. 8, NASA announced Feb. 28, 1969, as the planned launch date for Apollo 9.

Apollo 9 astronauts James A. McDivitt, front, David R. Scott, and Russell L. Schweickart depart crew quarters for the ride to Launch Pad 39A for emergency escape training Scott, left, Schweickart, and McDivitt in the White Room during the pad emergency escape drill Scott, left, McDivitt, and Schweickart pose with their mission patch following a press conference at Grumman Aircraft and Engineering Corporation in Bethpage, New York
Left: Apollo 9 astronauts James A. McDivitt, front, David R. Scott, and Russell L. Schweickart depart crew quarters for the ride to Launch Pad 39A for emergency escape training. Middle: Scott, left, Schweickart, and McDivitt in the White Room during the pad emergency escape drill. Right: Scott, left, McDivitt, and Schweickart pose with their mission patch following a press conference at Grumman Aircraft and Engineering Corporation in Bethpage, New York.

Workers at the pad immediately began to prepare the vehicle for flight, including software integration tests with the Mission Control Center at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston. On Jan. 15, the prime and backup crews conducted emergency egress training from their spacecraft at Launch Pad 39A. Launch controllers at KSC successfully completed the Flight Readiness Test, the final major overall test of the vehicle’s systems, between Jan. 19 and 22. During a Jan. 25 press conference at the Grumman Aircraft and Engineering Corporation in Bethpage, New York, manufacturer of the LM, the Apollo 9 astronauts provided reporters with an overview of their mission.

Apollo 10

Assuming Apollo 9 met its objectives and the LM proved space worthy in Earth orbit, in May Apollo 10 would repeat many of those tests in lunar orbit, including flying to within nine miles of the Moon’s surface.

Apollo 10 backup astronauts L. Gordon Cooper, front, and Edgar D. Mitchell arrive in the vacuum chamber in the Manned Spacecraft Operations Building (MSOB) at NASA’s Kennedy Space Center in Florida for a Lunar Module (LM) altitude test Engineers in the MSOB conduct a docking test between the LM and the Command Module (CM) docking test Engineers prepare the CM for an altitude test
Left: Apollo 10 backup astronauts L. Gordon Cooper, front, and Edgar D. Mitchell arrive in the vacuum chamber in the Manned Spacecraft Operations Building (MSOB) at NASA’s Kennedy Space Center in Florida for a Lunar Module (LM) altitude test. Middle: Engineers in the MSOB conduct a docking test between the LM and the Command Module (CM) docking test. Right: Engineers prepare the CM for an altitude test.

In November 1968, just six months before the planned launch date, NASA officially named the Apollo 10 crew. The prime crew consisted of Thomas P. Stafford, John W. Young, and Eugene A. Cernan. All had flown Gemini missions and had recently served as the Apollo 7 backup crew. L. Gordon Cooper, Donn F. Eisele, and Edgar D. Mitchell served as their backups.

In High Bay 2 of the Vehicle Assembly Building at NASA’s Kennedy Space Center (KSC) in Florida, the three stages of the Apollo 10 Saturn V await the arrival of the spacecraft In KSC’s Manned Spacecraft Operations Building (MSOB), workers remove the Lunar Module (LM) from an altitude chamber Workers in the MSOB lower the LM onto the base of the Spacecraft LM Adapter (SLA) After installing the main engine bell, workers lift the Command and Service Module for mating with the SLA
Left: In High Bay 2 of the Vehicle Assembly Building at NASA’s Kennedy Space Center (KSC) in Florida, the three stages of the Apollo 10 Saturn V await the arrival of the spacecraft. Middle left: In KSC’s Manned Spacecraft Operations Building (MSOB), workers remove the Lunar Module (LM) from an altitude chamber. Middle right: Workers in the MSOB lower the LM onto the base of the Spacecraft LM Adapter (SLA). Right: After installing the main engine bell, workers lift the Command and Service Module for mating with the SLA.

In the VAB’s High Bay 2, workers had completed stacking the Apollo 10 Saturn V’s three stages by the final days of 1968, while their colleagues prepared to roll Apollo 9’s rocket to the pad a few days later. In the nearby Manned Spacecraft Operations Building (MSOB), prime and backup crews completed altitude tests of the LM in December and workers conducted a docking test between the LM and the CM. On Jan. 16, Stafford, Young, and Cernan completed their altitude test of the CM, followed by Cooper, Eisele, and Mitchell the next day. Workers removed the spacecraft from the altitude chamber in preparation for its rollover to the VAB in early February for stacking onto the rocket.

Apollo 11

Assuming Apollo 9 and 10 accomplished their objectives, Apollo 11 would attempt the first Moon landing in July. Should Apollo 11 not succeed, NASA would try again with Apollo 12 in September and even Apollo 13 in November or December. Spacecraft and rocket manufacturers continued building components to meet that aggressive schedule.

Apollo 11 crew of Edwin E. “Buzz” Aldrin, left, Neil A. Armstrong, and Michael Collins
Apollo 11 crew of Edwin E. “Buzz” Aldrin, left, Neil A. Armstrong, and Michael Collins.

On Jan. 9, a mere six months before the planned launch date, NASA formally announced the Apollo 11 crew, the second all-veteran three-person crew after Apollo 10 – and the last all-veteran crew until STS-26 in 1988. The next day, NASA introduced the Apollo 11 crew during a press conference at MSC. The prime crew consisted of Neil A. Armstrong, Michael Collins, and Edwin E. “Buzz” Aldrin. Each astronaut had flown one Gemini mission. Armstrong and Aldrin had served on the backup crew for Apollo 8 while Collins was initially a member of the prime Apollo 8 crew until a bone spur in his neck requiring surgery sidelined him. He fully recovered from the operation, and NASA included him in the Apollo 11 crew. The Apollo 11 backup crew consisted of James A. Lovell, William A. Anders, and Fred W. Haise. Lovell and Anders had just completed the Apollo 8 lunar orbit mission with Haise a backup crew member on that flight. When Anders announced that he would retire from NASA in August 1969 to join the National Space Council, Thomas K. “Ken” Mattingly began training in parallel with Anders in case the mission slipped past that date.

The Lunar Module for Apollo 11 arrives at NASA’s Kennedy Space Center (KSC) in Florida The Apollo 11 Command Module, left, and Service Module, in KSC’s Manned Spacecraft Operations Building shortly after their arrival The S-IVB third stage for Apollo 11’s Saturn V rocket arrives at KSC
Left: The Lunar Module for Apollo 11 arrives at NASA’s Kennedy Space Center (KSC) in Florida. Middle: The Apollo 11 Command Module, left, and Service Module, in KSC’s Manned Spacecraft Operations Building shortly after their arrival. Right: The S-IVB third stage for Apollo 11’s Saturn V rocket arrives at KSC.

Hardware began to arrive at KSC for Apollo 11. With the Apollo 10 CSM still undergoing testing in the MSOB, the Apollo 11 LM’s ascent and descent stages arrived Jan. 8 and 12, respectively, followed by the CM and SM on Jan. 23. Workers in the MSOB prepared the spacecraft for vacuum chamber testing. The Saturn V’s S-IVB third stage arrived on Jan. 19. Workers trucked it to the VAB where it awaited the arrival of the first two stages, scheduled for February.

Lunar Receiving Laboratory

Schematic of the Lunar Receiving Laboratory (LRL) showing its major functional areas A mockup Command Module in the spacecraft storage area, part of the Crew Reception Area, in the LRL
Left:  Schematic of the Lunar Receiving Laboratory (LRL) showing its major functional areas.  Right:  A mockup Command Module in the spacecraft storage area, part of the Crew Reception Area, in the LRL.

With the Moon landing possibly just six months away, NASA continued to prepare key facilities designed to receive astronauts returning from the Moon. The 83,000-square-foot Lunar Receiving Laboratory (LRL), residing in MSC’s Building 37, was specially designed and built to isolate the astronauts, their spacecraft, and lunar samples to prevent back-contamination of the Earth by any possible lunar micro-organisms, and to maintain the lunar samples in as pristine a condition as possible. The building was completed in 1967, and over the next year, workers outfitted its laboratories and other facilities. A 10-day simulation in the facility in November 1968 found some deficiencies that NASA addressed promptly. On Jan. 23, 1969, workers brought a mockup Apollo CM into the LRL’s spacecraft storage area for fit checks.

Workers at the Norfolk Naval Air Station in Virginia hoist the Mobile Quarantine facility (MQF) onto the USS Guadalcanal The flexible tunnel set up between the MQF and a mockup Command Module Workers in Norfolk load the MQF onto a C-141 cargo plane for the return flight to Ellington Air Force Base in Houston
Left: Workers at the Norfolk Naval Air Station in Virginia hoist the Mobile Quarantine facility (MQF) onto the USS Guadalcanal. Middle: The flexible tunnel set up between the MQF and a mockup Command Module. Right: Workers in Norfolk load the MQF onto a C-141 cargo plane for the return flight to Ellington Air Force Base in Houston.

An integral component of the back-contamination prevention process was the Mobile Quarantine Facility (MQF). Following lunar landing missions, the MQF housed astronauts and support personnel from their arrival onboard the prime recovery ship shortly after splashdown through transport to the LRL. Under contract to NASA, Melpar, Inc., of Falls Church, Virginia, converted four 35-foot Airstream trailers into MQFs, delivering the first unit in March 1968 and the last three in the spring of 1969. The first unit was used extensively for testing, with lessons learned incorporated into the later models. On Jan. 21, 1969, workers loaded the MQF aboard a U.S. Air Force C-141 cargo plane at Ellington Air Force Base near MSC to transport it to the Norfolk Naval Air Station in Virginia. Six recovery specialists from MSC spent 10 days inside the MQF, first aboard the helicopter landing-platform USS Guadalcanal (LPH-7), including attaching a flexible tunnel to a boilerplate Apollo CM, and then aboard the destroyer USS Fox (DLG-33). The overall exercise, successfully completed on Feb. 3, tested all MQF systems aboard ships and aircraft to simulate recovery operations after a lunar landing mission.

To be continued …

With special thanks to Ed Hengeveld for imagery expertise.

News from around the world in January 1969:

Jan. 7 – Congress doubles the President’s salary from $100,000 to $200,000 a year.

Jan. 9 – First test flight of the Franco-British Concorde supersonic jetliner in Bristol, U.K.

Jan. 12 – In Super Bowl III, played in Miami’s Orange Bowl, the New York Jets beat the Baltimore Colts 16 to 7.

Jan. 16 – The Soviet Union conducts the first docking between two crewed spacecraft and the first crew transfer by spacewalking cosmonauts during the Soyuz 4 and 5 missions.

Jan. 20 – Richard M. Nixon inaugurated as the 37th U.S. President.

Jan. 30 – The Beatles perform their last live gig, a 42-minute concert on the rooftop of Apple Corps Headquarters in London.

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      Meteor Showers
      Unfortunately, one of the three major meteor showers of the year, the Geminids (004 GEM), will peak the morning of December 14, with the light of the nearly full Moon interfering. According to the International Meteor Organization, observers south of about 30 degrees north might be able to see these meteors for an hour or so between moonset and the first light of dawn (although the radiant for this meteor shower is at 33 degrees north latitude, so observers too far south of the equator will also have limited visibility). In a good year, this shower can produce 150 visible meteors per hour under ideal conditions, but this will not be a good year. For the Washington, DC area the MeteorActive app predicts that at about 2 AM EST on the morning of December 14, under bright suburban sky conditions, the peak rate from the Geminids and all other background sources might reach 20 meteors per hour.
      If the weather cooperates by being clear with no clouds or hazes and you do go looking for meteors, try to find a place as far as possible from light sources that has a clear view of a wide expanse of the sky. Give your eyes plenty of time to adapt to the dark. Your color vision (cone cells), concentrated in the center of your field of view, will adapt to darkness in about 10 minutes. Your more sensitive night vision rod cells will continue to improve for an hour or more (with most of the improvement in the first 35 to 45 minutes). The more sensitive your eyes are, the more chance you will have of seeing meteors. Since some meteors are faint, you will tend to see more meteors from the “corner of your eye.” Even a short exposure to light (from passing car headlights, etc.) will start the adaptation over again (so no turning on a light or your cell phone to check what time it is).
      In addition, a number of relatively minor meteor showers will peak during this lunar cycle. The light of the waning Moon will interfere with the Leonids (013 LEO) on November 17, α-Monocerotids (246 AMO) on November 21, and November Orionids (250 NOO) on November 28. The Phoenicids (254 PHO), best seen from the Southern Hemisphere, may peak around December 1. Models predict low rates and faint meteors this year but not much is known about this meteor shower. Most years the rates are low, but as reported by the International Meteor Organization, significant activity was observed in 2014. Once, in 1956, the Phoenicids reached an estimated rate of 100 visible meteors per hour. Another Southern Hemisphere shower is the Puppid-Velids (301 PUP), expected to peak sometime around December 4 at about 10 meteors per hour (under ideal conditions). The Monocerotids (019 MON) and σ-Hydrids (016 HYD) are both expected to peak on December 9 at 3 meteors per hour and 7 meteors per hour, respectively. These rates are low enough that seeing them from our light-polluted urban areas will be unlikely.
      Evening Sky Highlights
      On the evening of Friday, November 15 (the evening of the full Moon), as twilight ends (at 5:55 PM EST), the rising Moon will be 14 degrees above the east-northeastern horizon with the Pleiades star cluster 5 degrees to the lower left. The brightest planet in the sky will be Venus at 12 degrees above the southwestern horizon. Next in brightness will be Mercury at less than a degree above the west-southwestern horizon. Saturn will be 38 degrees above the south-southeastern horizon. Comet C/2023 A3 (Tsuchinshan-ATLAS) will be 39 degrees above the west-southwestern horizon, with its current brightness curve predicting it will have faded to magnitude 8, too faint to see with the unaided eye. The bright star closest to overhead will be Deneb at 79 degrees above the northwestern horizon. Deneb (visual magnitude 1.3) is the 19th brightest star in our night sky and is the brightest star in the constellation Cygnus the swan. One of the three bright stars of the “Summer Triangle” (along with Vega and Altair). Deneb is about 20 times more massive than our Sun but has used up its hydrogen, becoming a blue-white supergiant about 200 times the diameter of the Sun. If Deneb were where our Sun is, it would extend to about the orbit of the Earth. Deneb is about 2,600 light years from us.
      As this lunar cycle progresses, Saturn and the background of stars will appear to shift westward each evening (as the Earth moves around the Sun). Bright Venus will shift to the left and higher in the sky along the southwestern horizon. Mercury, shining brighter than Saturn, will initially shift left along the southwestern horizon until November 19, after which it will shift to the right. On November 22 Jupiter will join the planets Venus, Mercury and Saturn in the sky as twilight ends, shining brighter than Mercury. November 24 will be the last evening Mercury will be above the horizon as evening twilight ends, although it will remain visible in the glow of dusk for a few more evenings as it dims and shifts towards its passage between the Earth and the Sun on December 5. Jupiter will be at its closest and brightest for the year on December 7. The waxing Moon will pass by Venus on December 4, Saturn on December 7, and the Pleiades on December 13.
      By the evening of Saturday, December 14 (the start of the night of the December 15 full Moon), as twilight ends (at 5:50 PM EST), the rising Moon will be 19 degrees above the east-northeastern horizon with bright planet Jupiter 6 degrees to the right and the bright star Aldebaran father to the right. The brightest planet visible will be Venus at 21 degrees above the southwestern horizon. Next in brightness will be Jupiter. Saturn will be 43 degrees above the southern horizon. The bright star closest to overhead will still be Deneb at 61 degrees above the west-northwestern horizon.
      Morning Sky Highlights
      On the morning of Friday, November 15 (the morning of the full Moon after next), as twilight begins (at 5:51 AM EST), the setting full Moon will be 7 degrees above the west-northwestern horizon. The brightest planet in the sky will be Jupiter at 35 degrees above the western horizon. Mars will be at 68 degrees above the southwestern horizon. Comet C/2024 S1 (ATLAS) will not be visible, even with a telescope, as it broke apart into pieces too small to see as it passed its closest to the Sun on October 28. The bright star appearing closest to overhead will be Pollux at 69 degrees above the west-southwestern horizon (higher than Mars by about a half degree). Pollux is the 17th brightest star in our night sky and the brighter of the twin stars in the constellation Gemini. It is an orange tinted star about 34 lightyears from Earth. Pollux is not quite twice the mass of our Sun but about 9 times the diameter and 33 times the brightness.
      As this lunar cycle progresses, Jupiter, Mars, and the background of stars will appear to shift westward each evening, with Mars passing near the Beehive star cluster in early December. The waning Moon will pass by the Pleiades star cluster on November 16, Jupiter on November 17, Mars and Pollux on November 20, appear on the other side of Mars on November 21, Regulus on November 22 and 23, and Spica on November 27 (passing in front of Spica for parts of the USA and Canada). Jupiter will be at its closest and brightest on December 7, rising around sunset and setting around sunrise. December 12 will be the first morning Mercury will be above the east-southeastern horizon as morning twilight begins, though it will be visible in the glow of dawn for a few days before.
      By the morning of Sunday, December 15 (the morning of the full Moon after next), as twilight begins (at 6:16 AM EST), the setting full Moon will be 15 degrees above the west-northwestern horizon. The brightest planet in the sky will be Jupiter, appearing below the Moon at 5 degrees above the horizon. Second in brightness will be Mars at 46 degrees above the western horizon, then Mercury at 4 degrees above the east-southeastern horizon. The bright star appearing closest to overhead will be Regulus at 55 degrees above the southwestern horizon, with Arcturus a close second at 52 degrees above the east-southeastern horizon. Regulus is the 21st brightest star in our night sky and the brightest star in the constellation Leo the lion. The Arabic name for Regulus translates as “the heart of the lion.” Although we see Regulus as a single star, it is actually four stars (two pairs of stars orbiting each other). Regulus is about 79 light years from us. Arcturus is the brightest star in the constellation Boötes the herdsman or plowman and the 4th brightest star in our night sky. It is 36.7 light years from us. While it has about the same mass as our Sun, it is about 2.6 billion years older and has used up its core hydrogen, becoming a red giant 25 times the size and 170 times the brightness of our Sun. One way to identify Arcturus in the night sky is to start at the Big Dipper, then follow the arc of the handle as it “arcs towards Arcturus.”
      Detailed Daily Guide
      Here for your reference is a day-by-day listing of celestial events between now and the full Moon on December 15, 2024. The times and angles are based on the location of NASA Headquarters in Washington, DC, and some of these details may differ for where you are (I use parentheses to indicate times specific to the DC area). If your latitude is significantly different than 39 degrees north (and especially for my Southern Hemisphere readers), I recommend using an astronomy app set for your location or a star-watching guide from a local observatory, news outlet, or astronomy club.
      Thursday morning, November 14, at 6:18 EST, the Moon will be at perigee, its closest to the Earth for this orbit.
      As mentioned above, the full Moon will be Friday afternoon, November 15, 2024, at 4:29 PM EST. This will be early Saturday morning from Kamchatka and Fiji Time eastwards to the International Date Line. It will be the last of four consecutive supermoons. The Pleiades star cluster will appear near the full Moon. The Moon will appear full for about 3 days around this time, from a few hours before sunrise Thursday morning to a few hours before sunrise Sunday morning.
      Friday evening into Saturday morning, November 15 to 16, the Pleiades star cluster will appear near the full Moon. This may best be viewed with binoculars, as the brightness of the full Moon may make it hard to see the stars in this star cluster. As evening twilight ends (at 5:55 PM EST), the Pleiades will appear 5 degrees to the lower left of the full Moon. By the time the Moon reaches its highest for the night (Saturday morning at 12:07 AM), the Pleiades will be 2 degrees to the upper left. The Moon will pass in front of the Pleiades in the early morning hours. By the time morning twilight begins (at 5:52 AM) the Pleiades will be a degree to the lower right of the Moon.
      Saturday, November 16, will be when the planet Mercury reaches its greatest angular separation from the Sun as seen from the Earth for this apparition (called greatest elongation). Because the angle between the line from the Sun to Mercury and the line of the horizon changes with the seasons, the date when Mercury and the Sun are farthest apart as seen from the Earth is not always the same as when Mercury appears highest above the southwestern horizon as evening twilight ends, which will occur three evenings later, on November 19.
      Saturday night into Sunday morning, November 16 to 17, the planet Uranus will be at its closest and brightest for the year, called “opposition” because on Saturday night it will be opposite the Earth from the Sun. At opposition Uranus can be bright enough to see with the unaided eye (under very clear, dark sky conditions). From our light-polluted urban locations you will need binoculars or a telescope.
      Also on Saturday night into Sunday morning, November 16 to 17, the planet Jupiter will appear near the full Moon. As Jupiter rises on the east-northeastern horizon (at 6:14 PM EST) it will be 10 degrees to the lower left of the Moon. The Moon will reach its highest for the night about 7 hours later (at 1:09 AM), with Jupiter 7.5 degrees to the lower left. By the time morning twilight begins (at 5:52 AM) Jupiter will be 6 degrees to the left of the Moon.
      Tuesday night into Wednesday morning, November 19 to 20, the bright star Pollux and the bright planet Mars will appear near the waning gibbous Moon. As the Moon rises on the northeastern horizon (at 8:20 PM EST), Pollux will be 2.5 degrees to the upper left of the Moon. By the time the Moon reaches its highest in the sky (at 4:11 AM) Pollux will be 5 degrees to the upper right of the Moon, with Mars 7.5 degrees to the lower left of the Moon, such that these three appear aligned. By the time morning twilight begins (at 5:55 AM) Mars will be 7 degrees to the upper left and Pollux 5.5 degrees to the lower right.
      Wednesday night into Thursday morning, November 20 to 21, the waning gibbous Moon will have shifted to the other side of Mars. As the Moon rises on the east-northeastern horizon (at 9:29 PM EST) Mars will be 4 degrees to the upper right of the Moon. By the time the Moon reaches its highest for the night (at 5:03 AM) Mars will be 7 degrees to the right of the Moon. Morning twilight will begin less than an hour later (at 5:56 AM) with Mars 7 degrees to the lower right of the Moon.
      Friday evening, November 22, will be the first evening the bright planet Jupiter will be above the east-northeastern horizon as evening twilight ends (at 5:51 PM EST).
      Also on Friday evening, the waning Moon will appear half-full as it reaches its last quarter at 8:28 PM EST (when we can’t see it).
      Friday night into Saturday morning, November 22 to 23, the bright star Regulus will appear near the waning half-Moon. As Regulus rises on the east-northeastern horizon (at 11:29 PM EST) it will be 9 degrees below the Moon, with Mars farther to the upper right and Pollux beyond Mars. By the time the Moon reaches its highest for the night (at 5:49 AM) Regulus will be 7 degrees to the lower left, and morning twilight will begin 8 minutes later (at 5:57 AM).
      Saturday night into Sunday morning, November 23 to 24, the waning crescent Moon will have shifted to the other side of Regulus. When the Moon rises on the east-northeastern horizon (at 11:38 PM EST) Regulus will be 4 degrees to the upper right of the Moon. The pair will separate as the night progresses. By the time morning twilight begins (at 5:58 AM) Regulus will be 6.5 degrees to the upper right of the Moon.
      Sunday evening, November 24, will be the last evening the planet Mercury will be above the west-southwestern horizon as evening twilight ends, although it should remain visible in the glow of dusk before twilight ends for a few more evenings as it dims and shifts towards its passage between the Earth and the Sun on December 5.
      Tuesday morning, November 26, at 6:57 AM EST, the Moon will be at apogee, its farthest from the Earth for this orbit.
      On Wednesday morning, November 27, the bright star Spica will appear near the waning crescent Moon. As Spica rises on the east-southeastern horizon (at 3:41 AM EST) it will be a degree below the Moon. As morning progresses the Moon will shift towards Spica, and for much of the Eastern USA and Canada the Moon will block Spica from view. See http://www.lunar-occultations.com/iota/bstar/1127zc1925.htm for a map and information on the areas that will be able to see this eclipse. Times will vary by location, but for the Washington, DC area, Spica will vanish behind the illuminated limb of the Moon at 5:34 AM and the Moon will still be blocking Spica from sight as morning twilight begins at 6:02 AM.
      Early Sunday morning, December 1, at 1:22 AM EST, will be the new Moon, when the Moon passes between the Earth and the Sun and will not be visible from the Earth.
      The day of or the day after the New Moon marks the start of the new month for most moon-based calendars. The eleventh month of the Chinese year of the Dragon starts on Sunday, December 1. Sundown on Sunday, December 1, marks the start of Kislev in the Hebrew calendar. Hanukkah will begin towards the end of Kislev. In the Islamic calendar the months traditionally start with the first sighting of the waxing crescent Moon. Many Muslim communities now follow the Umm al-Qura Calendar of Saudi Arabia, which uses astronomical calculations to start months in a more predictable way. Using this calendar, sundown on Sunday, December 1, will probably mark the beginning of Jumādā ath-Thāniyah, also known as Jumādā al-ʾĀkhirah.
      Wednesday evening, December 4, the bright planet Venus will appear 3 degrees to the upper right of the waxing crescent Moon. The Moon will be 15 degrees above the southwestern horizon as evening twilight ends (at 5:49 PM EST). The Moon will set 2 hours later (at 7:46 PM).
      Thursday evening, December 5, the planet Mercury will be passing between the Earth and the Sun as seen from the Earth, called inferior conjunction. Planets that orbit inside of the orbit of Earth can have two types of conjunctions with the Sun, inferior (when passing between the Earth and the Sun) and superior (when passing on the far side of the Sun as seen from the Earth). Mercury will be shifting from the evening sky to the morning sky and will begin emerging from the glow of dawn on the eastern horizon in less than a week.
      Saturday afternoon, December 7, the planet Jupiter will be at its closest and brightest for the year, called “opposition” because it will be opposite the Earth from the Sun, effectively a “full” Jupiter. Jupiter will be 12 degrees above the east-northeastern horizon as evening twilight ends (at 5:49 PM EST), will reach its highest in the sky right around midnight (11:59 PM), and will be 11 degrees above the west-northwestern horizon as morning twilight begins (Sunday morning at 6:11 AM). Only planets that orbit farther from the Sun than the Earth can be seen at opposition.
      Saturday evening, December 7, the planet Saturn will appear to the upper left of the waxing crescent Moon. They will be 6 degrees apart as evening twilight ends (at 5:49 PM EST). Saturn will appear to shift clockwise and closer to the Moon, so that by the time the Moon sets 5.5 hours later (at 11:18 PM) Saturn will be 3.5 degrees above the Moon on the west-southwestern horizon. For a swath in the Pacific Ocean off the coast of Asia the Moon will actually block Saturn from view, see http://lunar-occultations.com/iota/planets/1208saturn.htm for a map and information on the locations that can see this eclipse.
      Sunday morning, December 8, the Moon will appear half-full as it reaches its first quarter at 10:27 AM EST (when we can’t see it).
      Thursday morning, December 12, will be the first morning the planet Mercury will be above the east-southeastern horizon as morning twilight begins (at 6:14 AM EST).
      Thursday morning, December 12, at 8:18 AM EST, the Moon will be at perigee, its closest to the Earth for this orbit.
      Friday evening into Saturday morning, December 13 to 14, the Pleiades star cluster will appear near the full Moon. This may best be viewed with binoculars, as the brightness of the full Moon may make it hard to see the stars in this star cluster. As evening twilight ends (at 5:50 PM EST), the Pleiades will appear 4 degrees to the upper right of the full Moon. By the time the Moon reaches its highest for the night (at 10:49 PM), the Pleiades will be 6 degrees to the right. By about 2 AM the Pleiades will be 8 degrees to the lower right of the Moon and they will continue to separate as the morning progresses.
      As mentioned above, one of the three major meteor showers of the year, the Geminids (004 GEM), will peak Saturday morning, December 14. The light of the nearly full Moon will interfere. In a good year, this shower can produce 150 visible meteors per hour under ideal conditions, but this will not be a good year. For the Washington, DC area the MeteorActive app predicts that at about 2 AM EST on the morning of December 14, under bright suburban sky conditions, the peak rate from the Geminids and all other background sources might reach 20 meteors per hour. See the meteor summary above for suggestions for meteor viewing.
      Saturday morning, December 14, the full Moon, the bright planet Jupiter, and the bright star Aldebaran will form a triangle. As Aldebaran sets on the west-northwestern horizon (at 6:10 AM EST) it will be 9 degrees to the lower left of the Moon with Jupiter 7 degrees to the upper left of the Moon. Morning twilight will begin 6 minutes later.
      Saturday evening, December 15, the full Moon will have shifted to the other side of Jupiter. Jupiter will be 6 degrees to the right of the Moon as evening twilight ends (at 5:50 PM EST) and the pair will separate as the night progresses.  
      The full Moon after next will be Sunday morning, December 15, 2024, at 4:02 AM EST. This will be Saturday evening from Alaska Time westwards to the International Date Line. The Moon will appear full for about 3 days around this time, from Friday evening through Monday morning, making this a full Moon weekend.
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    • NASA
      40 Years Ago: STS-51A – “The Ace Repo Company”
      By NASA
      Successfully deployed from the space shuttle Challenger during the February 1984 STS-41B mission, the Westar 6 and Palapa B2 communications satellites ended up in incorrect orbits due to failures of their upper stage rockets. During STS-51A in November 1984, Discovery’s second trip into space, the crew of Commander Frederick H. “Rick” Hauck, Pilot David M. Walker, and Mission Specialists Joseph P. Allen, Anna L. Fisher, and Dale A. Gardner worked as a team to not only deploy two new satellites but also to retrieve the two wayward but otherwise healthy satellites for return to Earth. Hauck and Walker piloted Discovery to rendezvous with each satellite in turn, Allen and Gardner retrieved them during two spacewalks, and Fisher grappled and placed them in the payload bay for return to Earth. After refurbishment, both satellites returned to space.

      Left: The STS-51A crew of Dale A. Gardner, left, David M. Walker, Anna L. Fisher, Frederick “Rick” H. Hauck, and Joseph P. Allen. Right: The STS-51A crew patch.
      NASA originally designated Hauck, Walker, Allen, Fisher, and Gardner as a crew in November 1983 and assigned them to STS-41H, a mission aboard Challenger planned for late September 1984 to either deploy the second Tracking and Data Relay Satellite (TDRS) or fly a classified payload for the Department of Defense. Due to ongoing problems with the Inertial Upper Stage that failed to put the first TDRS satellite in its correct orbit during STS-6, NASA canceled STS-41H and shifted Hauck’s crew to STS-51A. In February 1984, an agreement between NASA and the Canadian government added an as-yet unnamed Canadian payload specialist to the STS-51A crew. Managers later named the Canadian as Marc Garneau and reassigned him to STS-41G.
      A shuffling of payloads following the STS-41D launch abort resulted in STS-51A now deploying the Anik D2 satellite for Canada and Leasat 1 (also known as Syncom IV-1) for the U.S. Navy. By early August, the launch date had slipped to Nov. 2, with NASA considering the possibility of retrieving the two wayward satellites from STS-41B, officially adding that task on Aug. 13. NASA selected Allen in 1967 as one of 11 scientist-astronauts, while the rest of the crew hail from the Class of 1978. Hauck, on his second mission after serving as pilot on STS-7, has the distinction as the first from his class to command a shuttle mission. Allen and Gardner had each flown one previous mission, STS-5 and STS-8, respectively, while for Walker and Fisher STS-51A represented their first flight. Fisher has the distinction as the first mother in space. 

      Left: After its arrival from the Orbiter Processing Facility, workers in the Vehicle Assembly Building (VAB) prepare to lift Discovery for mating with an External Tank (ET) and Solid Rocket Boosters (SRBs). Middle: Workers lift Discovery to stack it with the ET and SRBs. Right: The completed stack prepares to leave the VAB for the rollout to Launch Pad 39A.
      Discovery arrived back at NASA’s Kennedy Space Center (KSC) in Florida on Sept. 10, returning from Edwards Air Force Base in California following the STS-41D mission. Workers towed it to the Orbiter Processing Facility (OPF) the next day to begin the process of refurbishing it for STS-51A. On Oct. 18, they rolled it over to the Vehicle Assembly Building (VAB), for stacking with an External Tank and twin Solid Rocket Boosters.

      At NASA’s Kennedy Space Center in Florida, space shuttle Discovery rolls out to Launch Pad 39A, with the Saturn V rocket on display in the foreground.
      The completed stack rolled out to Launch Pad 39A on Oct. 23. Two days later, the five-member STS-51A crew participated in the Terminal Countdown Demonstration Test, essentially a dress rehearsal for the actual countdown to launch. The crew returned to KSC on Nov. 5, the day the countdown began for a planned Nov. 7 launch. High upper-level winds that day forced a one-day delay.

      Left: STS-51A astronaut Dale A. Gardner trains for the capture of a satellite using the Apogee Kick Motor Capture Device. Middle: Astronaut Anna L. Fisher trains to use the Canadian-built Remote Manipulator System, or robotic arm. Right: As part of the Terminal Countdown Demonstration Test, the STS-51A astronauts practice rapid evacuation from the launch pad.
      Following deployment from Challenger during STS-41B, the upper stages of both the Westar 6 and Palapa B2 satellites malfunctioned, leaving them in non-useable 160-by-600-mile-high orbits instead of the intended 22,300-mile-high geostationary orbits required for their normal operations. While both satellites remained healthy, their own thrusters could not boost them to the proper orbits. NASA devised a plan to have astronauts retrieve the satellites during spacewalks using the jetpack known as the Manned Maneuvering Unit (MMU), after which the shuttle’s Canadian-built Remote Manipulator System (RMS) or robot arm would grapple them and place them into the cargo bay for return to Earth. Astronauts had demonstrated the capability of the MMU during the STS-41C Solar Max satellite repair mission in April 1984 and NASA felt confident of its ability to capture and return Westar and Palapa. 
      In the weeks prior to STS-51A, ground controllers lowered the orbits of both satellites and reduced their spin rates from 50 to 1 rpm to enable capture by the shuttle astronauts. Engineers at NASA’s Johnson Space Center in Houston developed the Apogee Kick Motor Capture Device (ACD), otherwise known as the stinger due to its appearance, to allow an astronaut to capture the satellites while flying the MMU. Once relocated over the payload bay, a second astronaut would remove the satellite’s omnidirectional antenna with pruning shears and install an Antenna Bridge Structure (ABS) with a grapple fixture over the satellite’s main antenna dish. Allen would fly the MMU to capture Palapa, then he would switch roles with Gardner who would capture Westar. Fisher would use the RMS to grapple the satellites by this second fixture and lower them into specially built cradles to secure them into the payload bay.

      Left: The STS-51A crew leaves crew quarters on their way to Launch Pad 39A. Middle: Liftoff of Discovery on the STS-51A mission. Right: View inside Discovery’s payload bay shortly after orbital insertion – the top of Anik D2 is visible, with Leasat 1 hidden behind it.
      Space shuttle Discovery roared off KSC’s Launch Pad 39A on Nov. 8, 1984, to begin the STS-51A mission and mark the orbiter’s first return to space. For Gardner, launch day coincided with his 36th birthday. The launch took place just 26 days after the landing of the previous mission, STS-41G, a then record-breaking turnaround time between shuttle flights. Eight and a half minutes after liftoff, Discovery and its five-member crew reached space and shortly thereafter settled into a 182-by-172-mile-high initial orbit. As their first order of business, the crew checked out the RMS to ensure its functionality for the satellite captures later in the mission. They also performed the first rendezvous burn to begin the approach to the Palapa satellite. The crew then settled down for its first night’s sleep in orbit.

      Left: Nighttime deploy of the Anik D2 satellite. Middle: Deploy of the Leasat 1 satellite. Right: Leasat 1 as it departs from Discovery.
      The primary activity of the second flight day involved Allen deploying the 2,727-pound Anik D2 satellite via a spring ejection mechanism, occurring on time and with no issues. The crew also circularized the shuttle’s orbit at 186 miles. The next day, Gardner deployed the 17,000-pound Leasat 1 using the Frisbee style mechanism used to deploy the first Leasat during STS-41D two months earlier. With the satellite deployments complete, the crew began to focus on the rendezvous maneuvers to bring them close to the Palapa B2 satellite while Allen and Gardner verified the functionality of their spacesuits. On flight day 4, the astronauts reduced the pressure inside the shuttle from 14.7 pounds per square inch (psi) to 10.2 psi in order to prevent the spacewalking astronauts from developing the bends inside the spacesuits that operated at 4.3 psi.

      Left: During the first spacewalk, Jospeh P. Allen captures the Palapa B2 satellite. Middle: Anna L. Fisher grasps Allen and Palapa with the Remote Manipulator System, or robotic arm. Right: Allen, left, and Dale A. Gardner prepare to place Palapa in its cradle in the payload bay.
      On the fifth mission day, after Hauck and Walker piloted Discovery to within 35 feet of Palapa, Allen and Gardner exited the airlock to begin the spacewalk portion of the satellite capture. Allen donned the MMU mounted on the side wall of the cargo bay, attached the stinger to its arms, and flew out to Palapa. Once there, he inserted the stinger into the satellite’s Apogee Kick Motor bell and using the MMU’s attitude control system stopped Palapa’s spin.
      Fisher then steered the RMS to capture a grapple fixture mounted on the stinger between Allen and the satellite. She then maneuvered them over the payload bay where Gardner waited to remove its omnidirectional antenna and install the bridge structure. However, Gardner could not attach the ABS to the satellite due to an unexpected clearance issue on the satellite. Using a backup plan, Allen undocked from the stinger, leaving it attached to the satellite as well as the RMS, and stowed the MMU in the payload bay. With Allen now holding the satellite by its antenna, Gardner attached an adaptor to the bottom end of the satellite to secure it in its cradle in the payload bay. This plan worked and Allen and Gardner completed the spacewalk in exactly six hours.

      Left: Dale A. Gardner flies the Manned Maneuvering Unit to capture Westar 6 during the second spacewalk. Middle: Anna L. Fisher operates the Remote Manipulator System from Discovery’s aft flight deck. Right: Gardner, left, and Joseph P. Allen maneuver Westar prior to placing it in its cradle in the payload bay.
      Between the two spacewalk days, the crew serviced the spacesuits, conducted routine maintenance on the shuttle, and prepared for the second rendezvous, this time to retrieve Westar. Allen and Gardner switched roles for the second spacewalk on flight day seven, with Gardner flying the MMU to capture Westar. The astronauts repeated the procedure from the first spacewalk, except for not removing the omni antenna so they could use it as a handhold. With Westar secured in the payload bay, Gardner and Allen completed the second spacewalk in 5 hours and 42 minutes.

      Left: Dale A. Gardner, left, and Joseph P. Allen pose at the end of the Remote Manipulator System controlled by Anna L. Fisher, holding a For Sale sign above the two retrieved satellites secured in Discovery’s payload bay. Middle: Inflight photo of the STS-51A crew after the successful satellite retrievals. Right: View inside Discovery’s payload bay shortly before the deorbit burn, with Westar 6 in the foreground and Palapa B2 behind it.
      During their final full day in space, Discovery’s crew repressurized the shuttle’s cabin to 14.7 psi and tidied the cabin in preparation for reentry. On Nov. 16, the astronauts closed the payload bay doors and fired the Orbital Maneuvering System engines to begin the descent back to Earth. Hauck guided Discovery to a smooth landing at KSC, completing a flight of 7 days, 23 hours, and 45 minutes. The crew had traveled nearly 3.3 million miles and completed 127 orbits around the Earth. The next day, workers towed Discovery to the OPF to begin preparing it for its next flight, STS-51C in January 1985.

      Left: Discovery streaks over Houston on its way to land at NASA’s Kennedy Space Center (KSC) in Florida. Middle: Discovery moments before touchdown at KSC. Right: NASA officials greet the STS-51A astronauts as they exit Discovery.
      As a postscript, STS-51A marked the last flight to use the MMUs, and the last untethered spacewalks until 1994 when STS-64 astronauts tested the Simplified Aid for EVA Rescue (SAFER). All subsequent spacewalks on the space shuttle and the International Space Station used safety tethers, with the SAFER as a backup in case a crew member disconnects from the vehicle.

      Left: In the Orbiter Processing Facility at NASA’s Kennedy Space Center in Florida, workers inspect the Westar 6, left, and Palapa B2 satellites in Discovery’s payload bay. Right: The STS-51A crew, with Lloyd’s of London representative Stephen Merritt, sitting at right, during their visit to London.
      On Dec. 7, 1984, in a ceremony at the White House, President Ronald W. Reagan presented the STS-51A crew with the Lloyd’s of London – the company had insured the two satellites they returned to Earth – Silver Medal for Meritorious Salvage Operations. Fisher has the distinction as only the second woman to receive that award. In February 1985, Lloyd’s flew the crew to London on the Concorde for a week of activities, including addressing the Lloyd’s underwriters and tea with Prince Charles at Kensington Palace.
      Hong Kong-based AsiaSat purchased the Westar 6 satellite, refurbished it, and relaunched it as AsiaSat 1 on April 7, 1990, on a Chinese CZ-3 rocket. Title to the Palapa B2 satellite returned to Indonesia after its relaunch as Palapa B2R on April 13, 1990, aboard a Delta rocket.
      Read recollections of the STS-51A mission by Hauck, Allen, and Fisher in their oral histories with the JSC History Office. Enjoy the crew’s narration of a video about the STS-51A mission.
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    • NASA
      NASA-Funded Study Examines Tidal Effects on Planet and Moon Interiors
      By NASA
      2 min read
      NASA-Funded Study Examines Tidal Effects on Planet and Moon Interiors
      NASA-supported scientists have developed a new method to compute how tides affect the interiors of planets and moons. Importantly, the new study looks at the effects of body tides on objects that don’t have a perfectly spherical interior structure, which is an assumption of most previous models.
      The puzzling, fascinating surface of Jupiter’s icy moon Europa looms large in this newly-reprocessed color view, made from images taken by NASA’s Galileo spacecraft in the late 1990s. This is the color view of Europa from Galileo that shows the largest portion of the moon’s surface at the highest resolution. NASA/JPL-Caltech/SETI Institute Body tides refer to the deformations experienced by celestial bodies when they gravitationally interact with other objects. Think of how the powerful gravity of Jupiter tugs on its moon Europa. Because Europa’s orbit isn’t circular, the crushing squeeze of Jupiter’s gravity on the moon varies as it travels along its orbit.  When Europa is at its closest to Jupiter, the planet’s gravity is felt the most. The energy of this deformation is what heats up Europa’s interior, allowing an ocean of liquid water to exist beneath the moon’s icy surface.
      “The same is true for Saturn’s moon Enceladus.” says co-author Alexander Berne of CalTech in Pasadena and an affiliate at NASA’s Jet Propulsion Laboratory in Southern California. “Enceladus has an ice shell that is expected to be much more non-spherically symmetric than that of Europa.”
      The body tides experienced by celestial bodies can affect how the worlds evolve over time and, in cases like Europa and Enceladus, their potential habitability for life as we know it. The new study provides a means to more accurately estimate how tidal forces affect planetary interiors.
      In this movie Europa is seen in a cutaway view through two cycles of its 3.5 day orbit about the giant planet Jupiter. Like Earth, Europa is thought to have an iron core, a rocky mantle and a surface ocean of salty water. Unlike on Earth, however, this ocean is deep enough to cover the whole moon, and being far from the sun, the ocean surface is globally frozen over. Europa’s orbit is eccentric, which means as it travels around Jupiter, large tides, raised by Jupiter, rise and fall. Jupiter’s position relative to Europa is also seen to librate, or wobble, with the same period. This tidal kneading causes frictional heating within Europa, much in the same way a paper clip bent back and forth can get hot to the touch, as illustrated by the red glow in the interior of Europa’s rocky mantle and in the lower, warmer part of its ice shell. This tidal heating is what keeps Europa’s ocean liquid and could prove critical to the survival of simple organisms within the ocean, if they exist. The giant planet Jupiter is now shown to be rotating from west to east, though more slowly than its actual rate. NASA/JPL-Caltech The paper also discusses how the results of the study could help scientists interpret observations made by missions to a variety of different worlds, ranging from Mercury to the Moon to the outer planets of our solar system.
      The study, “A Spectral Method to Compute the Tides of Laterally Heterogeneous Bodies,” was published in The Planetary Science Journal. 
      For more information on NASA’s Astrobiology Program, visit:
      https://science.nasa.gov/astrobiology
      -end-
      Karen Fox / Molly Wasser
      Headquarters, Washington
      202-358-1600
      karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov 
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