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Friday, March 29, 2019

Dragon 2 (SpaceX)

From Wikipedia, the free encyclopedia

SpaceX Dragon 2
SpaceX Crew Dragon (More cropped).jpg
Artistic rendition of a Crew Dragon 2 approaching the International Space Station (ISS)

ManufacturerSpaceX
Country of originUnited States
Operator
ApplicationsISS crew and cargo transport

Specifications
Design life
  • 1 week (free flight)
  • 210 Days 
Dry mass9,525 kg (20,999 lb)
Payload capacity
  • 6,000 kg (13,000 lb) to orbit
  • 3,000 kg (6,600 lb) return cargo
  • 800 kg (1,800 lb) disposed cargo
Crew capacity7
Dimensions
  • Diameter: 4 m (13 ft)
  • Height: 8.1 m (27 ft) (with trunk)
  • Sidewall angle: 15 degrees
Volume
  • 9.3 m3 (330 cu ft) pressurized
  • 12.1 m3 (430 cu ft) unpressurized

Production
StatusTesting
Built2 (1 test article, 1 production)
Launched1
First launchMarch 2, 2019

Related spacecraft
Derived fromSpaceX Dragon

Dragon 2 is a class of reusable spacecraft developed and manufactured by American aerospace manufacturer SpaceX, conceived as the successor to the Dragon cargo spacecraft. The spacecraft are designed for launches atop a Falcon 9 Block 5 rocket and a splashdown return. In comparison to its predecessor, it has larger windows, new flight computers and avionics, redesigned solar arrays, and a modified outer mold line. The spacecraft is used in two variants – Crew Dragon, a human-rated capsule capable of carrying up to seven astronauts, and Cargo Dragon, an updated replacement for the original Dragon. Cargo Dragon capsules are repurposed flown Crew Dragon capsules. Crew Dragon is uniquely equipped with a set of four side-mounted thruster pods with two SuperDraco engines each, which serve as a launch escape system. Both variants have been contracted for use with logistical operations of the International Space Station (ISS) under Commercial Resupply Services 2 (CRS2) and the Commercial Crew Program.

Development on Dragon 2 began as DragonRider in 2010, when NASA began searching for private operators for crewed flights to the ISS under the Commercial Crew Development program. Its design was publicly unveiled in May 2014, and in October 2014 was selected alongside Boeing's CST-100 Starliner to be developed for flight under the program. Considered by NASA as the least expensive option, US$2.6 billion was awarded to SpaceX to continue development of the spacecraft, in contrast to the US$4.2 billion awarded to Boeing. Crew Dragon's first non-piloted test flight to the ISS launched in March 2019, and its first crewed flight to the ISS is planned to occur in July 2019. Cargo Dragon was also selected in January 2016 alongside Northrop Grumman Innovation Systems' Cygnus and Sierra Nevada Corporation's Dream Chaser for cargo delivery flights under CRS2 contracts. SpaceX's initial CRS2 mission with the Cargo Dragon is slated to occur in August 2020 after SpaceX's final CRS mission with the original Dragon spacecraft, which is expected to launch no earlier than January 2020.

Development and variants

2012 DragonRider mockup, showing the launch escape system engines mounted on the outside of the capsule, when the design was not yet final.
 
Depictions of the Crew Dragon's 2014 design from various angles. Visible changes that occurred since then include the removal of the hatch and back windows.
 
The DM-1 Dragon 2 capsule at SpaceX's LC-39A Horizontal Integration Facility.
 
Depictions of the Crew Dragon's 2019 design as in DM-1 mission
 
Depictions of the Crew Dragon's 2019 design as in DM-1 mission
 
Dragon 2 has two variants: Crew Dragon and Cargo Dragon. Crew Dragon was initially called DragonRider and it was intended from the beginning to support a crew of seven or a combination of crew and cargo. It was planned to be able to perform fully autonomous rendezvous and docking with manual override ability; and was designed to use the NASA Docking System (NDS) to dock to the ISS. For typical missions, DragonRider would remain docked to the ISS for a period of 180 days, but would be designed to be able to do so for 210 days, the same as the Russian Soyuz spacecraft. From the earliest design concepts which were publicly released in 2010, SpaceX planned to use an integrated pusher launch escape system for the Dragon spacecraft, claiming several advantages over the tractor detachable tower approach used on most prior crewed spacecraft. These advantages included the provision for crew escape all the way to orbit, reusability of the escape system, improved crew safety due to eliminating a stage separation, and the ability to use the escape engines during landings for a precise solid earth landing of the capsule.

SpaceX originally intended to certify their propulsive landing scheme, in parallel with the parachute-to-water-landing method for Dragon 2, with the goal to hold to the development schedule and "ensure U.S. crew transportation safely and reliably in 2017." SpaceX announced that "land landing will become the baseline for the early post-certification missions" while precision water landing under parachutes was proposed to NASA as "the baseline return and recovery approach for the first few flights of Crew Dragon." Thus the parachute system was initially anticipated to be only a backup system; due to the cancellation of propulsive landing, however, the parachute system will be used for all landings. As of 2011, the Paragon Space Development Corporation was assisting in developing DragonRider's life support system. In 2012, SpaceX was in talks with Orbital Outfitters about developing space suits to wear during launch and re-entry.

At a NASA news conference on May 18, 2012, SpaceX confirmed again that their target launch price for crewed Dragon flights is $160 million, or $20 million per seat if the maximum crew of 7 is aboard, and if NASA orders at least four DragonRider flights per year. This contrasts with the 2014 Soyuz launch price of $76,000,000 per seat for NASA astronauts. The spacecraft's design was unveiled on May 29, 2014, during a press event at SpaceX headquarters in Hawthorne, California. In October 2014, NASA selected the Dragon spacecraft as one of the candidates to fly American astronauts to the International Space Station under the Commercial Crew Program. SpaceX plans to use the Falcon 9 Block 5 launch vehicle for launching Dragon 2.

Technical specifications

Dragon 2 includes the following features:
  • Reusability: partly reusable; can be flown multiple times, resulting in a significant cost reduction. Dragon 2 is only planned to fly crew on the first flight of a particular capsule, while future flights of a capsule would carry only cargo.
  • Capacity: 3,307 kilograms (7,291 lb) Cargo Dragon 2; seven astronauts Crew Dragon 2
  • Landing: four main parachutes for water landing; possibility of developing propulsive landing using the SuperDraco engines.
  • Engines (crewed variant): eight side-mounted SuperDraco engines, clustered in redundant pairs in four engine pods, with each engine able to produce 71 kilonewtons (16,000 lbf) of thrust Each pod—called a "quad" by SpaceX—contains two SuperDraco engines plus four Draco thrusters. "Nominally, only two quads are used for on-orbit propulsion with the Dracos and two quads are reserved for propulsive landing using the SuperDracos."
  • Engines (cargo variant): four Draco thrusters per pod with four pods, used for orbital maneuvers.
  • A 3D-printed rocket engine: the SuperDraco Engine combustion chamber is printed of Inconel, an alloy of nickel and iron, using a process of direct metal laser sintering. Engines are contained in a protective nacelle to prevent fault propagation if an engine fails.
  • Docking: able to autonomously dock to space stations. Dragon V1 used berthing, a non-autonomous means to attach to the ISS that was completed by use of the Canadarm2 robotic arm. Pilots retain the ability to park the spacecraft using manual controls if needed.
  • Propellant tanks: composite-carbon-overwrap titanium spherical tanks to hold the helium used to pressurize engines and also for the SuperDraco fuel and oxidizer
  • Thermal protection: SpaceX-developed SPAM backshell; updated third-generation PICA-X heat shield
  • Controls: static tablet-like computer and seats that swivel up to the touchscreens for optional crew control
  • Cabin depressurization protection: the spacecraft can be operated in full vacuum, and "the crew will wear SpaceX-designed space suits to protect them from a rapid cabin depressurization emergency event". Also, the spacecraft will be able to return safely if a leak occurs "of up to an equivalent orifice of 0.25 inches [6.35 mm] in diameter."
  • Movable ballast sled: to allow more precise attitude control of the spacecraft during the atmospheric entry phase of the return to Earth and more accurate control of the landing ellipse location.
  • Reusable nose cone: "protects the vessel and the docking adaptor during ascent and reentry"; pivots on a hinge to enable in-space docking, and returns to the covered position for reentry and future launches
  • Trunk: the third structural element of the spacecraft, which contains the solar arrays, heat-removal radiators, and will provide aerodynamic stability during emergency aborts.
The landing system was initially designed to accommodate three types of landing scenarios:
  • Propulsive landing, for vertical takeoff, vertical landing (VTVL)
  • Parachute landing, similar to prior American crewed space capsules
  • Parachute landing with propulsive assist, similar to that used by the Soyuz: "The whole landing system is designed so that it’s survivable if there’s no propulsive assist at all. So if you come down chutes only with the landing legs, we anticipate no crew injury. It’ll be kind of like landing in the Soyuz."
On July 19, 2017, Elon Musk announced that propulsive landing development had been halted and all landings would be under parachute followed by splashdown. The SuperDraco engines would still be used for emergency aborts, but there would be no landing legs. The effort to qualify propulsive landing for safety as well as the lack of technology commonalities with their ultimate Starship was given as a reason. However, pending approval from NASA, the SuperDraco engines can still be used for propulsive landings in case multiple parachutes fail.

The parachute system was fully redesigned from the one used in the prior Dragon capsule, due to the need to deploy the parachutes under a variety of launch abort scenarios.

Space suit

Dragon crew members will wear a custom space suit designed to protect them during rapid cabin depressurization. It is intended to be worn only inside a pressurized spacecraft for intravehicular activities (IVA type). For the SpX-DM1 test, a test dummy nicknamed Ripley was fitted with the spacesuit and sensors.

Planned space transport missions

Maiden flight of the Dragon 2 atop a Falcon 9.
 
Dragon has been designed to fulfill a set of mission requirements that will make the capsule useful to both commercial and government customers. SpaceX and Bigelow Aerospace are working together to support round-trip transport of commercial passengers to low Earth orbit (LEO) destinations such as the planned Bigelow Commercial Space Station. In that use, the full passenger capacity of seven passengers is planned to be used. SpaceX competed for a contract with NASA to deliver some number of specific crew-transport missions to the ISS under the third phase of the Commercial Crew Development program. In an August 2014 presentation, SpaceX revealed that if NASA chooses to use the Dragon 2 space capsule under a Commercial Crew Transportation Capability (CCtCap, Commercial Crew Development) contract, then only four of the seven possible seats would be used for carrying NASA-designated passengers to the ISS, as NASA would like to use the added payload mass and volume ability to carry pressurized cargo. Also, all NASA landings of Dragon 2 are planned to initially use the propulsive deceleration ability of the SuperDraco engines only for a propulsive assist right before final touchdown, and would otherwise use parachutes "all the way down."

On 16 September 2014, NASA announced that SpaceX, together with Boeing, has been selected to provide crew transport ability to ISS. SpaceX will receive $2.6 billion under this contract. NASA considers Dragon to be the least expensive proposal. Comparing the Dragon to the Boeing CST-100, NASA's William H. Gerstenmaier considers the CST-100 proposal the stronger of the two. In a departure from prior NASA practice during the first five decades of the space age, where NASA contracted with commercial firms to build spaceflight equipment and then NASA operated the spacecraft directly, NASA is purchasing space transport services from SpaceX with the Dragon 2 contract, and will leave the launch, transit, and operation of the spacecraft to SpaceX.

Crewed flights contracted to NASA

SpaceX has contracted to fly a number of crewed flights to low-Earth orbit (LEO) for the US space agency NASA. These flights are slated to begin no earlier than June 2019, with an automated test mission to the International Space Station (ISS) launched on March 2, 2019. In August 2018, NASA and SpaceX agreed on the loading procedures for propellants, vehicle fluids and crew. High-pressure helium will be loaded first, followed by the passengers approximately two hours prior to scheduled launch; the ground crew will then depart the launch pad and remove to a safe distance. The launch escape system will be activated approximately 40 minutes prior to launch, with propellant loading commencing several minutes later.

Flight testing

Abort and hover tests

Dragon 2 hover test (24159153709)
Pad Abort test of a Dragon 2 article on 6 May 2015 at Cape Canaveral SLC-40
 
SpaceX planned a series of four flight tests for the Dragon 2 that included both a "pad abort" test, an in-flight abort test, plus both an uncrewed robotic orbital flight to the ISS, and finally a 14-day crewed demonstration mission to the ISS, currently planned for 2019. In August 2014, it was announced that the pad abort test would occur in Florida, at SpaceX's leased pad at SLC-40, and the test was conducted successfully on 6 May 2015. Dragon landed safely in the ocean to the east of the launchpad 99 seconds later. While a flight-like Dragon 2 and trunk were used for the pad abort test, they rested atop a truss structure for the test rather than a full Falcon 9 rocket. A crash test dummy embedded with a suite of sensors was placed inside the test vehicle to record acceleration loads and forces at the crew seat, while the remaining six seats were loaded with weights to simulate full-passenger-load weight. The test objective was to demonstrate sufficient total impulse, thrust and controllability to conduct a safe pad abort. A fuel mixture ratio issue was detected after the flight in one of the eight SuperDraco engines, but did not materially affect the flight. On 24 November 2015, SpaceX conducted a test of Dragon 2's hovering abilities at the firm's rocket development facility in McGregor, Texas. In a video published by the firm, the spacecraft is shown suspended by a hoisting cable and igniting its SuperDraco engines. The capsule hovers in equilibrium for about 5 seconds, kept in balance by its 8 engines firing at reduced thrust to compensate exactly for gravity. The video shows the second test of the two-part milestone under NASA's Commercial Crew Development contract with SpaceX. The first test, a short firing of the engines intended to verify a healthy propulsion system, was completed two days earlier on 22 November. The test vehicle was the same capsule that performed the pad abort test earlier in 2015; it was nicknamed DragonFly.

SpaceX plans to conduct an in-flight abort test from Kennedy Space Center Launch Complex 39A in Florida after the first uncrewed orbital test flight and prior to the first crewed test flight. The test is planned to be conducted approximately in June 2019 with the refurbished capsule from the uncrewed test flight. Earlier, this test had been scheduled before the uncrewed orbital test, however, SpaceX and NASA consider it safer to use the more recently designed capsule rather than the older test article from the pad abort test. The Dragon 2 test capsule will be launched in a sub-orbital flight to conduct a separation and abort scenario in the troposphere at transonic velocities, at max. Q, where the vehicle experiences maximum aerodynamic pressure. The test objective is to demonstrate the ability to safely move away from the ascending rocket under the most challenging atmospheric conditions of the flight trajectory, imposing the worst structural stress of a real flight on the rocket and spacecraft. The capsule will then splash down in the ocean with traditional parachutes, possibly with assistance of its integrated thrusters to smooth the final moments of the descent. The in-flight abort capsule was originally planned to launch on F9R Dev2 before the Falcon 9 Full Thrust vehicle (and its densified propellants) made F9R Dev2 incompatible with both of SpaceX's active orbital launch pads. Then a special version of the Falcon 9 first stage with just three engines was prepared for this test and carried to the launch pad at Vandenberg in April 2015 to conduct a tanking test. It was erected on the revised and rebuilt transporter erector (TE) and fully loaded with propellants on 9 April 2015 to test both the vehicle and ground support equipment. Those plans were later scrapped, and the abort test will be performed using an entire Falcon 9 Block 5 rocket and will be used as a test of the fueling procedure in order to human-rate the Falcon 9 rocket for NASA's Commercial Crew Program.

Orbital flight tests

Crew Dragon 2 mockup (background) and the astronauts selected for its first two crewed missions (foreground), from left to right: Douglas Hurley, Robert Behnken, Michael Hopkins and Victor Glover.
 
In 2015, NASA named its first Commercial Crew astronaut cadre of four veteran astronauts to work with SpaceX and Boeing – Robert Behnken, Eric Boe, Sunita Williams, and Douglas Hurley. The SpX-DM2 mission will complete the last milestone of the Commercial Crew Development program, paving the way to starting commercial services under an upcoming ISS Crew Transportation Services contract. On August 3, 2018 NASA announced the crew for the DM-2 mission. The crew of two will be formed by NASA astronauts Bob Behnken and Doug Hurley. Behnken previously flew as mission specialist on the STS-123 and the STS-130 missions. Hurley previously flew as a pilot on the STS-127 mission and on the final Space Shuttle mission, the STS-135 mission.

The first orbital test of Crew Dragon 2 was an uncrewed mission, designated SpX-DM1 and launched March 2, 2019. The spacecraft tested the approach and automated docking procedures with the ISS, remained docked until March 8, 2019, then conducted the full re-entry, splashdown and recovery steps to qualify for a crewed mission. Life-support systems were monitored all along the test flight. The same capsule will be re-used in June for an in-flight abort test. As of February 2019, Dragon 2 is scheduled to carry its first crew of two NASA astronauts on a 14-day test-flight mission to the ISS in July 2019.

List of missions

List includes only completed or currently manifested missions. Launch dates are listed in UTC.
Mission Capsule № Launch date (UTC) Remarks Time at ISS (dd hh mm) Outcome
Dragon 2 pad abort test DragonFly 6 May 2015 Pad abort test, Cape Canaveral Air Force Station, Florida N/A Success
SpX-DM1 C201 2 March 2019 Uncrewed test flight of the Dragon 2 capsule; Docked 3 March 0851 UTC, Departed 8 March 0532 UTC 4:21:17 Success
Dragon 2 in-flight abort test C201 (reused capsule) June 2019 The in-flight abort test will be conducted with the refurbished capsule from the uncrewed test flight. N/A Planned
SpX-DM2 C203 July 2019 Crewed test flight of the Dragon 2 capsule, with two astronauts for two weeks
Planned
CCtCap Missions 1–6
2019 and after First operational crew transport mission with Dragon 2. Pending success of SpX-DM1 and SpX-DM2, NASA has awarded six missions with Dragon 2.0 to carry up to four astronauts and 220 pounds of cargo to the ISS as well as feature a lifeboat function to evacuate astronauts from ISS in case of an emergency.
Planned
CRS2 missions 1–6
2020–2024 NASA has awarded SpaceX six more cargo missions under the CRS2 contract. Those missions were originally scheduled to begin in 2019 but were delayed.
Planned

Philae (spacecraft)

From Wikipedia, the free encyclopedia

Philae
Philae lander (transparent bg).png
Illustration of Philae
Mission typeComet lander
OperatorEuropean Space Agency / DLR
COSPAR ID2004-006C
Websitewww.esa.int/rosetta
Mission durationPlanned: 1–6 weeks
Active: 12-14 November 2014
Hibernation: 15 November 2014 – 13 June 2015
Spacecraft properties
ManufacturerDLR / MPS / CNES / ASI
Launch mass100 kg (220 lb)
Payload mass21 kg (46 lb)
Dimensions1 × 1 × 0.8 m (3.3 × 3.3 × 2.6 ft)
Power32 watts at 3 AU
Start of mission
Launch date2 March 2004, 07:17 UTC
RocketAriane 5G+ V-158
Launch siteKourou ELA-3
ContractorArianespace
End of mission
Last contact9 July 2015, 18:07 UTC
67P/Churyumov–Gerasimenko lander
Landing date12 November 2014, 17:32 UTC
Landing siteAbydos
 
Philae is a robotic European Space Agency lander that accompanied the Rosetta spacecraft until it separated to land on comet 67P/Churyumov–Gerasimenko, ten years and eight months after departing Earth. On 12 November 2014, Philae touched down on the comet, but it bounced when its anchoring harpoons failed to deploy and a thruster designed to hold the probe to the surface did not fire. After bouncing off the surface twice, Philae achieved the first-ever "soft" (nondestructive) landing on a comet nucleus, although the lander's final, uncontrolled touchdown left it in a non-optimal location and orientation.

Despite the landing problems, the probe's instruments obtained the first images from a comet's surface. Several of the instruments on Philae made the first direct analysis of a comet, sending back data that will be analysed to determine the composition of the surface.

On 15 November 2014 Philae entered safe mode, or hibernation, after its batteries ran down due to reduced sunlight and an off-nominal spacecraft orientation at its unplanned landing site. Mission controllers hoped that additional sunlight on the solar panels might be sufficient to reboot the lander. Philae communicated sporadically with Rosetta from 13 June to 9 July 2015, but contact was then lost. The lander's location was identified to within a few tens of metres, but it was not seen. Philae, though silent, was finally identified unambiguously, lying on its side in a deep crack in the shadow of a cliff, in photographs taken by Rosetta on 2 September 2016 as the orbiter was sent on orbits closer to the comet. Knowledge of its precise location will help in interpretation of the images it had sent. On 30 September 2016, the Rosetta spacecraft ended its mission by crashing in the comet's Ma'at region.

The lander is named after the Philae obelisk, which bears a bilingual inscription and was used along with the Rosetta Stone to decipher Egyptian hieroglyphs. Philae was monitored and operated from DLR's Lander Control Center in Cologne, Germany.

Mission

Philae's mission was to land successfully on the surface of a comet, attach itself, and transmit data about the comet's composition. The Rosetta spacecraft and Philae lander were launched on an Ariane 5G+ rocket from French Guiana on 2 March 2004, 07:17 UTC, and travelled for 3,907 days (10.7 years) to Churyumov–Gerasimenko. Unlike the Deep Impact probe, which by design struck comet Tempel 1's nucleus on 4 July 2005, Philae is not an impactor. Some of the instruments on the lander were used for the first time as autonomous systems during the Mars flyby on 25 February 2007. CIVA, one of the camera systems, returned some images while the Rosetta instruments were powered down, while ROMAP took measurements of the Martian magnetosphere. Most of the other instruments need contact with the surface for analysis and stayed offline during the flyby. An optimistic estimate of mission length following touchdown was "four to five months".

Scientific goals

The goals of the scientific mission have been summarized as follows:
The scientific goals of its experiments focus on elemental, isotopic, molecular and mineralogical composition of the cometary material, the characterization of physical properties of the surface and subsurface material, the large-scale structure and the magnetic and plasma environment of the nucleus. In particular, surface and sub-surface samples will be acquired and sequentially analyzed by a suite of instruments. Measurements will be performed primarily during descent and along the first five days following touch-down.

Landing and surface operations

Depiction of Philae on Churyumov-Gerasimenko
 
Philae remained attached to the Rosetta spacecraft after rendezvousing with Churyumov–Gerasimenko on 6 August 2014. On 15 September 2014, ESA announced "Site J" on the smaller lobe of the comet as the lander's destination. Following an ESA public contest in October 2014, Site J was renamed Agilkia in honour of Agilkia Island.

A series of four Go/NoGo checks were performed on 11–12 November 2014. One of the final tests before detachment from Rosetta showed that the lander's cold-gas thruster was not working correctly, but the "Go" was given anyway, as it could not be repaired. Philae detached from Rosetta on 12 November 2014 at 08:35 UTC SCET.

Landing events

Rosetta signal received at ESOC in Darmstadt, Germany (20 January 2014)
 
Philae's landing signal was received by Earth communication stations at 16:03 UTC after a 28-minute delay. Unknown to mission scientists at that time, the lander had bounced. It began performing scientific measurements while slowly moving away from the comet and coming back down, confusing the science team. Further analysis showed that it bounced twice.

Philae's first contact with the comet occurred at 15:34:04 UTC SCET. The probe rebounded off the comet's surface at 38 cm/s (15 in/s) and rose to an altitude of approximately 1 km (0.62 mi). For perspective, had the lander exceeded about 44 cm/s (17 in/s), it would have escaped the comet's gravity. After detecting the touchdown, Philae's reaction wheel was automatically powered off, resulting in its momentum being transferred back into the lander. This caused the vehicle to begin rotating every 13 seconds. During this first bounce, at 16:20 UTC SCET, the lander is thought to have struck a surface prominence, which slowed its rotation to once every 24 seconds and sent the craft tumbling. Philae touched down a second time at 17:25:26 UTC SCET and rebounded at 3 cm/s (1.2 in/s). The lander came to a final stop on the surface at 17:31:17 UTC SCET. It sits in rough terrain, apparently in the shadow of a nearby cliff or crater wall, and is canted at an angle of around 30 degrees, but is otherwise undamaged. Its final location was determined initially by analysis of data from CONSERT in combination with the comet shape model based on images from the Rosetta orbiter, and later precisely by direct imaging from Rosetta.

An analysis of telemetry indicated that the initial impact was softer than expected, that the harpoons had not deployed, and that the thruster had not fired. The harpoon propulsion system contained 0.3 grams of nitrocellulose, which was shown by Copenhagen Suborbitals in 2013 to be unreliable in a vacuum.

Operations and communication loss

Philae's intended landing site Agilkia (Site J)
 
The primary battery was designed to power the instruments for about 60 hours. ESA expected that a secondary rechargeable battery would be partially filled by the solar panels attached to the outside of the lander, but the limited sunlight (90 minutes per 12.4-hour comet day) at the actual landing site was inadequate to maintain Philae's activities, at least in this phase of the comet's orbit.

On the morning of 14 November 2014, the battery charge was estimated to be only enough for continuing operations for the remainder of the day. After first obtaining data from instruments whose operation did not require mechanical movement, comprising about 80% of the planned initial science observations, both the MUPUS soil penetrator and the SD2 drill were commanded to deploy. Subsequently, MUPUS data as well as COSAC and Ptolemy data were returned. A final set of CONSERT data was also downlinked towards the end of operations. During the evening's transmission session, Philae was raised by 4 centimetres (1.6 in) and its body rotated 35 degrees to more favourably position the largest solar panel to capture the most sunlight in the future. Shortly afterwards, electrical power dwindled rapidly and all instruments were forced to shut down. The downlink rate slowed to a trickle before coming to a stop. Contact was lost on 15 November at 00:36 UTC.

The German Aerospace Center's lander manager Stephan Ulamec stated:
Prior to falling silent, the lander was able to transmit all science data gathered during the First Science Sequence ... This machine performed magnificently under tough conditions, and we can be fully proud of the incredible scientific success Philae has delivered.

Instrument results

Data from the SESAME instrument determined that, rather than being "soft and fluffy" as expected, Philae's first touchdown site held a large amount of water ice under a layer of granular material about 25 cm (9.8 in) deep. It found that the mechanical strength of the ice was high and that cometary activity in that region was low. At the final landing site, the MUPUS instrument was unable to hammer very far into the comet's surface, despite power being gradually increased. This area was determined to have the consistency of solid ice or pumice.

In the atmosphere of the comet, the COSAC instrument detected the presence of molecules containing carbon and hydrogen. Soil elements could not be assessed, because the lander was unable to drill into the comet surface, likely due to hard ice. The SD2 drill went through the necessary steps to deliver a surface sample to the COSAC instrument, but nothing entered the COSAC ovens.

Upon Philae's first touchdown on the comet's surface, COSAC measured material at the bottom of the vehicle, which was disturbed by the landing, while the Ptolemy instrument measured material at the top of the vehicle. Sixteen organic compounds were detected, four of which were seen for the first time on a comet, including acetamide, acetone, methyl isocyanate and propionaldehyde.

Reawakening and subsequent loss of communication

Comet Churyumov–Gerasimenko in September 2014 as imaged by Rosetta
 
On 13 June 2015 at 20:28 UTC, ground controllers received an 85-second transmission from Philae, forwarded by Rosetta, indicating that the lander was in good health and had sufficiently recharged its batteries to come out of safe mode. Philae sent historical data indicating that although it had been operating earlier than 13 June 2015, it had been unable to contact Rosetta before that date. The lander reported that it was operating with 24 watts of electrical power at −35 °C (−31 °F).

A new contact between Rosetta and Philae was confirmed on 19 June 2015. The first signal was received on the ground from Rosetta at 13:37 UTC, while a second signal was received at 13:54 UTC. These contacts lasted about two minutes each and delivered additional status data. By 26 June 2015, there had been a total of seven intermittent contacts between the lander and orbiter. There were two opportunities for contact between the two spacecraft each Earth day, but their duration and quality depended on the orientation of the transmitting antenna on Philae and the location of Rosetta along its trajectory around the comet. Similarly, as the comet rotated, Philae was not always in sunlight and thus not always generating enough power via its solar panels to receive and transmit signals. ESA controllers continued to try to establish a stable contact duration of at least 50 minutes.

Had Philae landed at the planned site of Agilkia in November 2014, its mission would probably have ended in March 2015 due to the higher temperatures of that location as solar heating increased. As of June 2015, Philae's key remaining experiment was to drill into the comet's surface to determine its chemical composition. Ground controllers sent commands to power up the CONSERT radar instrument on 5 July 2015, but received no immediate response from the lander. Confirmation was eventually received on 9 July, when the lander transmitted measurement data from the instrument.

Immediately after its reawakening, housekeeping data suggested that the lander's systems were healthy, and mission control uploaded commands for Rosetta to establish a new orbit and nadir so as to optimize communications, diagnostics, and enable new science investigations with Philae. However, controllers had difficulties establishing a stable communications connection with the lander. The situation was not helped by the need to keep Rosetta at a greater and safer distance from the comet as it became more active. The last communication was on 9 July 2015, and mission controllers were unable to instruct Philae to carry out new investigations. Subsequently, Philae failed to respond to further commands, and by January 2016, controllers acknowledged no further communications were likely.

On 27 July 2016, at 09:00 UTC, ESA switched off the Electrical Support System Processor Unit (ESS) onboard Rosetta, making further communications with Philae impossible.

Location

The lander was located on 2 September 2016 by the narrow-angle camera aboard Rosetta as it was slowly making its descent to the comet. The search for the lander had been on-going during the Rosetta mission, using telemetry data and comparison of pictures taken before and after the lander's touchdown, looking for signs of the lander's specific reflectivity.

The search area was narrowed down to the most promising candidate, which was confirmed by a picture taken at a distance of 2.7 km (1.7 mi), clearly showing the lander. The lander sits on its side wedged into a dark crevice of the comet, explaining the lack of electrical power and proper communication with the probe. Knowing its exact location provides information needed to put Philae's two days of science into proper context.

Design

Rosetta and Philae
 
The lander was designed to deploy from the main spacecraft body and descend from an orbit of 22.5 kilometres (14 mi) along a ballistic trajectory. It would touch down on the comet's surface at a velocity of around 1 metre per second (3.6 km/h; 2.2 mph). The legs were designed to dampen the initial impact to avoid bouncing as the comet's escape velocity is only around 1 m/s (3.6 km/h; 2.2 mph), and the impact energy was intended to drive ice screws into the surface. Philae was to then fire a harpoon into the surface at 70 m/s (250 km/h; 160 mph) to anchor itself. A thruster on top of Philae was to have fired to lessen the bounce upon impact and to reduce the recoil from harpoon firing. During the landing, the harpoons did not fire and the thruster failed to operate, leading to a multiple-contact landing.

Communications with Earth used the Rosetta orbiter as a relay station to reduce the electrical power needed. The mission duration on the surface was planned to be at least one week, but an extended mission lasting months was considered possible. 

The main structure of the lander is made from carbon fiber, shaped into a plate maintaining mechanical stability, a platform for the science instruments, and a hexagonal "sandwich" to connect all the parts. The total mass is about 100 kilograms (220 lb). Its exterior is covered with solar cells for power generation.

The Rosetta mission was originally planned to rendezvous with the comet 46P/Wirtanen. A failure in a previous Ariane 5 launch vehicle closed the launch window to reach the comet with the same rocket. It resulted in a change in target to the comet 67P/Churyumov–Gerasimenko. The larger mass of Churyumov–Gerasimenko and the resulting increased impact velocity required that the landing gear of the lander be strengthened.

Spacecraft component Mass
Structure 18.0 kg 39.7 lb
Thermal control system 3.9 kg 8.6 lb
Power system 12.2 kg 27 lb
Active descent system 4.1 kg 9.0 lb
Reaction wheel 2.9 kg 6.4 lb
Landing gear 10.0 kg 22 lb
Anchoring system 1.4 kg 3.1 lb
Central data management system 2.9 kg 6.4 lb
Telecommunications system 2.4 kg 5.3 lb
Common electronics box 9.8 kg 22 lb
Mechanical support system, harness, balancing mass 3.6 kg 7.9 lb
Scientific payload 26.7 kg 59 lb
Sum 97.9 kg 216 lb

Power management

Philae's power management was planned for two phases. In the first phase, the lander operated solely on battery power. In the second phase, it was to run on backup batteries recharged by solar cells.

The power subsystem comprises two batteries: a non-rechargeable primary 1000 watt-hour battery to provide power for the first 60 hours and a secondary 140 watt-hour battery recharged by the solar panels to be used after the primary is exhausted. The solar panels cover 2.2 square metres (24 sq ft) and were designed to deliver up to 32 watts at a distance of 3 AU from the Sun.

Instruments

Philae's instruments
 
The science payload of the lander consists of ten instruments totalling 26.7 kilograms (59 lb), making up just over one quarter of the mass of the lander.
APXS
The Alpha Particle X-ray Spectrometer detects alpha particles and X-rays, which provide information on the elemental composition of the comet's surface. The instrument is an improved version of the APXS on the Mars Pathfinder.
CIVA
The Comet Nucleus Infrared and Visible Analyser (sometimes given as ÇIVA) is a group of seven identical cameras used to take panoramic pictures of the surface plus a visible-light microscope and an infrared spectrometer. The panoramic cameras (CIVA-P) are arranged on the sides of the lander at 60° intervals: five mono imagers and two others making up a stereo imager. Each camera has a 1024×1024 pixel CCD detector. The microscope and spectrometer (CIVA-M) are mounted on the base of the lander, and are used to analyse the composition, texture and albedo (reflectivity) of samples collected from the surface.
CONSERT
The COmet Nucleus Sounding Experiment by Radiowave Transmission used electromagnetic wave propagation to determine the comet's internal structure. A radar on Rosetta transmitted a signal through the nucleus to be received by a detector on Philae.
COSAC
The COmetary SAmpling and Composition instrument is a combined gas chromatograph and time-of-flight mass spectrometer to perform analysis of soil samples and determine the content of volatile components.
MUPUS
The MUlti-PUrpose Sensors for Surface and Sub-Surface Science instrument measured the density, thermal and mechanical properties of the comet's surface.
Ptolemy
An instrument measuring stable isotope ratios of key volatiles on the comet's nucleus.
ROLIS
The Rosetta Lander Imaging System is a CCD camera used to obtain high-resolution images during descent and stereo panoramic images of areas sampled by other instruments. The CCD detector consists of 1024×1024 pixels.
ROMAP
The Rosetta Lander Magnetometer and Plasma Monitor is a magnetometer and plasma sensor to study the nucleus' magnetic field and its interactions with the solar wind.
SD2
The Sampling, Drilling and Distribution system obtains soil samples from the comet and transfers them to the Ptolemy, COSAC, and CIVA instruments for in-situ analysis. SD2 contains four primary subsystems: drill, ovens, carousel, and volume checker. The drill system, made of steel and titanium, is capable of drilling to a depth of 230 mm (9.1 in), deploying a probe to collect samples, and delivering samples to the ovens. There are a total of 26 platinum ovens to heat samples—10 medium temperature ovens at 180 °C (356 °F) and 16 high temperature ovens at 800 °C (1,470 °F)—and one oven to clear the drill bit for reuse. The ovens are mounted on a rotating carousel that delivers the active oven to the appropriate instrument. The electromechanical volume checker determines how much material was deposited into an oven, and may be used to evenly distribute material on CIVA's optical windows. Development of SD2 was led by the Italian Space Agency with contributions by prime contractor Tecnospazio S.p.A (now Selex ES S.p.A.) in charge of the system design and overall integration; the Italian company Tecnomare S.p.A., owned by Eni S.p.A., in charge of the design, development, and testing of the drilling/sampling tool and the volume checker; Media Lario; and Dallara. The instrument's principal investigator is Amalia Ercoli-Finzi (Politecnico di Milano).
SESAME
The Surface Electric Sounding and Acoustic Monitoring Experiments used three instruments to measure properties of the comet's outer layers. The Cometary Acoustic Sounding Surface Experiment (CASSE) measures the way in which sound travels through the surface. The Permittivity Probe (PP) investigates its electrical characteristics, and the Dust Impact Monitor (DIM) measures dust falling back to the surface.

International contributions

Austria
The Austrian Space Research Institute developed the lander's anchor and two sensors within MUPUS, which are integrated into the anchor tips.
Belgium
The Belgian Institute for Space Aeronomy (BIRA) cooperated with different partners to build one of the sensors (DFMS) of the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) instrument. The Belgian Institute for Space Aeronomy (BIRA) and Royal Observatory of Belgium (ROB) provided information about the space weather conditions at Rosetta to support the landing of Philae. The main concern was solar proton events.
Canada
Two Canadian companies played a role in the mission. SED Systems, located on the University of Saskatchewan campus in Saskatoon, built three ground stations that were used to communicate with the Rosetta spacecraft. ADGA-RHEA Group of Ottawa provided MOIS (Manufacturing and Operating Information Systems) software which supported the procedures and command sequences operations software.
Finland
The Finnish Meteorological Institute provided the memory of the Command, Data and Management System (CDMS) and the Permittivity Probe (PP).
France
The French Space Agency, together with some scientific laboratories (IAS, SA, LPG, LISA) provided the system's overall engineering, radiocommunications, battery assembly, CONSERT, CIVA and the ground segment (overall engineering and development/operation of the Scientific Operation & Navigation Centre).
Germany
The German Space Agency (DLR) has provided the structure, thermal subsystem, flywheel, the Active Descent System (procured by DLR but made in Switzerland), ROLIS, downward-looking camera, SESAME, acoustic sounding and seismic instrument for Philae. It has also managed the project and did the level product assurance. The University of Münster built MUPUS (it was designed and built in Space Research Centre of Polish Academy of Sciences ) and the Braunschweig University of Technology the ROMAP instrument. The Max Planck Institute for Solar System Research made the payload engineering, eject mechanism, landing gear, anchoring harpoon, central computer, COSAC, APXS and other subsystems.
Hungary
The Command and Data Management Subsystem (CDMS) designed in the Wigner Research Centre for Physics of the Hungarian Academy of Sciences jointly with the Space and Ground Facilities Ltd. (a spin-off company of the Wigner Research Centre for Physics). The Power Subsystem (PSS) designed in the Department of Broadband Infocommunications and Electromagnetic Theory at Budapest University of Technology and Economics. CDMS is the fault tolerant central computer of the lander, while PSS assures that the power coming from the batteries and solar arrays are properly handled, controls battery charging and manages the onboard power distribution.
Ireland
Captec Ltd., based in Malahide, provided the independent validation of mission critical software (independent software validation facility or SVF) and developed the software for the communications interface between the orbiter and the lander. Captec also provided engineering support to the prime contractor for the launch activities at Kourou. Space Technology Ireland Ltd. at Maynooth University has designed, constructed and tested the Electrical Support System Processor Unit (ESS) for the Rosetta mission. ESS stores, transmits and provides decoding for the command streams passing from the spacecraft to the lander and handles the data streams coming back from the scientific experiments on the lander to the spacecraft.
Italy
The Italian Space Agency (ASI) developed the SD2 instrument and the photovoltaic assembly. Italian Alenia Space was involved in the assembly, integration and testing of the probe, as well as several mechanical and electrical ground support equipment. The company also built the probe's S-band and X-band digital transponder, used for communications with Earth.
Netherlands
Moog Bradford (Heerle, The Netherlands) provided the Active Descent System, which guided and propelled the lander down to its landing zone. To accomplish the ADS, a strategic industrial team was formed with Bleuler-Baumer Mechanik in Switzerland.
Poland
The Space Research Centre of the Polish Academy of Sciences built the Multi-Purpose Sensors for Surface and Subsurface Science (MUPUS).
Spain
The GMV Spanish division has been responsible for the maintenance of the calculation tools to calculate the criteria of lighting and visibility necessary to decide the point of landing on the comet, as well as the possible trajectories of decline of the Philae module. Other important Spanish companies or educational institutions that have been contributed are as follows: INTA, Airbus Defence and Space Spanish division, other small companies also participated in subcontracted packages in structural mechanics and thermal control like AASpace (former Space Contact), and the Universidad Politécnica de Madrid.
Switzerland
The Swiss Centre for Electronics and Microtechnology developed CIVA.
United Kingdom
The Open University and the Rutherford Appleton Laboratory (RAL) developed PTOLEMY. RAL also constructed the blankets that kept the lander warm throughout its mission. Surrey Satellites Technology Ltd. (SSTL) constructed the momentum wheel for the lander. It stabilised the module during the descent and landing phases. Manufacturer e2v supplied the CIVA and Rolis camera systems used to film the descent and take images of samples, as well as three other camera systems.

Media coverage

The landing was featured heavily in social media, with the lander having an official Twitter account portraying a personification of the spacecraft. The hashtag "#CometLanding" gained widespread traction. A Livestream of the control centres was set up, as were multiple official and unofficial events around the world to follow Philae's landing on Churyumov–Gerasimenko. Various instruments on Philae were given their own Twitter accounts to announce news and science results.

Popular culture

Vangelis composed the music for the trio of music videos released by ESA to celebrate the first-ever attempted soft landing on a comet by ESA's Rosetta mission.

On 12 November 2014, the search engine Google featured a Google Doodle of Philae on its home page. On 31 December 2014, Google featured Philae again as part of its New Year's Eve 2014 Doodle.

Online comic author Randall Munroe wrote a live updating strip on his website xkcd on the day of the landing.

Education

From Wikipedia, the free encyclopedia https://en.wikipedia.org/wiki/Education Education is the transmissio...