This article provides a timeline of theCassini–Huygens mission (commonly calledCassini).Cassini was a collaboration between theUnited States'NASA, theEuropean Space Agency ("ESA"), and theItalian Space Agency ("ASI") to send a probe to study the Saturnian system, including the planet, itsrings, and itsnatural satellites.^[1][2] TheFlagship-classuncrewedrobotic spacecraft comprised both NASA'sCassini probe, and ESA'sHuygenslander which was designed to land on Saturn's largest moon,Titan.Cassini was the fourthspace probe to visitSaturn and the first to enter its orbit. The craft were named after astronomersGiovanni Cassini andChristiaan Huygens.

Launched aboard aTitan IVB/Centaur on 15 October 1997,Cassini had a nearly 20-year life span, with 13 of these years spent orbiting Saturn.^[3] The voyage to Saturn includedflybys ofVenus (April 1998 and June 1999),Earth (August 1999), theasteroid2685 Masursky, andJupiter (December 2000). The probesentered orbit on 1 July 2004, and the mission ended on 15 September 2017, whenCassini flew into Saturn's upper atmosphere^[4][5] in order to prevent any risk of contaminating Saturn's moons, some of which have active environments that could potentially bear life.^[6][7] The mission is widely perceived to have succeeded beyond expectations.Cassini-Huygens has been described by NASA'sPlanetary Science Division Director as a "mission of firsts",^[8] that has revolutionized human understanding of the Saturnian system, including its moons andrings, and our understanding of where life might be found in theSolar System.

Cassini's primary mission lasted for four years, from June 2004 to May 2008. The mission was extended for another two years until September 2010, under the name ofCassini Equinox Mission. The mission was extended a second and final time with theCassini Solstice Mission, lasting until the spacecraft's destruction in September 2017.

TheHuygens module traveled withCassini until its separation from the probe on 25 December 2004; it was successfully landed byparachute onTitan on 14 January 2005. It successfully returned data to Earth for around 90 minutes, using the orbiter as a relay. This was the firstlanding ever accomplished in the outerSolar System and the first landing on a moon other than our own.

At the end of its mission, theCassini spacecraft executed the "Grand Finale" of its mission: several risky passes through the gaps between Saturn and Saturn's inner rings.^[1][2] The purpose of this phase was to maximizeCassini's scientific outcome before the spacecraft was destroyed.^[9] Theatmospheric entry ofCassini effectively ended the mission, although data analysis and production is still ongoing.

15 October 1997 01:43Pacific Daylight Time (PDT) –Cassini launched at 08:43 UTC insideTitan IVB/Centaur rocket atCape Canaveral.

26 April 1998 06:52 PDT –Gravity-assisted flyby ofVenus at 284 km, receiving a boost in speed of about 7 kilometers per second.^[10]

3 December 1998 22:06 PST –Cassini fired its main rocket engine for 90 minutes, setting the spacecraft on course for its second Venus flyby in 1999. The engine burn slowed the spacecraft by close to 450 meters per second (about 1,006 miles per hour) relative to the Sun.Cassini's speed went from 67,860 kilometers per hour (42,168 miles per hour) at the start of the maneuver to 66,240 kilometers per hour (41,161 miles per hour) at the end of the engine firing.^[11]

24 June 1999 13:30 PDT – Gravity-assisted flyby ofVenus at 623 km.^[12]

18 August 1999 03:28 UTC − Gravity-assisted flyby of Earth. An hour 20 minutes before closest approach,Cassini made the closest approach to the Moon at 377,000 km, and took a series of calibration images.The spacecraft flew past Earth at a distance of 1,171 kilometers (728 mi), passing most closely above the eastern South Pacific at23°30′S128°30′W / 23.5°S 128.5°W /-23.5; -128.5.Cassini received a 5.5-kilometer-per-second (about 12,000-mile-per-hour) boost in velocity.^[13]

23 January 2000 – flyby ofAsteroid2685 Masursky around 10:00 UTC.Cassini took images^[14] 5 to 7 hours before at 1.6 million km distance and estimated a diameter of 15 to 20 km.

30 December 2000 10:05 UTC − Gravity-assisted flyby ofJupiter.Cassini was at its closest point (9.7 million kilometres, 137 Jovian radii) to Jupiter at this date, and performed many scientific measurements.^[15] It also produced the most detailed global color portrait of Jupiter ever produced (seen on the right); the smallest visible features are approximately 60 km (37 mi) across.

30 May 2001 – During thecoast phase between Jupiter and Saturn, it was noticed that "haze" became visible in the pictures taken by the narrow-angle camera ofCassini. This was first seen when a picture of the starMaia in thePleiades was taken after a routine heating period.

23 July 2002 – In late January, a test was performed to remove the "haze" from the narrow-angle camera lens by heating it. Warming the camera to 4 degrees Celsius (39 degrees Fahrenheit) for eight days produced positive results. Later, the heating was extended to 60 days, and a picture of the starSpica showed an improvement of more than 90 percent compared to before the heating period. On 9 July, a picture showed that the removal procedure was completed successfully, which was announced on 23 July.^[16]

10 October 2003 – TheCassini science team announced the results of a test ofEinstein's theory ofgravity, using radio signals from theCassini probe. The researchers observed afrequency shift in the radio waves to and from the space craft, as those signals traveled close to theSun. Past tests were in agreement with the theoretical predictions with an accuracy of one part in one thousand. TheCassini experiment improved this to about 20 parts in a million, with the data still supporting Einstein's theory.

27 February 2004 – A new, high-resolution picture of Saturn taken byCassini on 9 February was released, and it was noted that mission scientists were puzzled by the fact that no "spokes" in Saturn's ring are visible. These dark structures in the "B" section of the ring had been discovered in pictures taken by theVoyager probe in 1981.^[17] Another picture, in infrared light, taken on 16 February shows cloud height differences and the same disturbance visible throughout the 1990s inHubble Space Telescope images.^[18]

12 March 2004 – Pictures taken on 23 February do show a feature discovered byVoyager: Clumps in the outer "F"-ring. What could not be ascertained at the time was the exact lifetime of these clumps, and it is hoped thatCassini will provide conclusive data about this question. The first set of pictures shows a set of "clumps" moving along the "F" ring.^[19]

26 March 2004 – TheCassini science team published the first sequence of pictures of Saturn showing clouds moving at high speed around the planet. Using a filter to better see water haze on top of the dense cloud cover, motions in the equatorial and southern regions are clearly visible.^[20] The pictures were taken during the days from 15 to 19 February.

8 April 2004 – The first "long-term" observation of cloud dynamics in Saturn's atmosphere were published by mission scientists. A set of pictures shows two storms in the southern latitudes merge during a period from 19 to 20 March. Both storms had a diameter of about 1,000 km (620 mi) before they merged.

15 April 2004 – NASA announced that two moons discovered by Voyager 1 were sighted again byCassini in pictures taken on 10 March:Prometheus andPandora. These are no ordinary moons, but their gravitational effects on the "F" ring led scientists to call them "shepherd moons". They fascinate all researchers interested in the dynamics of the ring system, because their orbits are close enough that they interact with each other in achaotic manner. They have a history of defying predictions of their orbits. One ofCassini's missions will be to monitor the movements of these bodies closely.

18 May 2004 –Cassini entered the Saturn system. The gravitational pull of Saturn began to overtake the influence of the Sun.

20 May 2004 – The first picture of Titan with better resolution than any Earth-based observation was released. It was taken 5 May from a distance of 29.3 million kilometers (18.2 million miles).

27 May 2004 – TCM-20, thePhoebe approach TCM (Trajectory Correction Maneuver) was executed at 22:26:00 UTC. This was a 5-minute and 56 second burn of the main engine, which was not used since December 1998. It therefore doubled as a "dress rehearsal" for the 96 minute burn during "Saturn Orbit Insertion" (SOI). However, TCM-20 was mainly designed to change Cassini's velocity by 34.7 m/s (78 mph), setting up a flyby of the moon Phoebe 11 June.

11 June 2004 –Cassini flew by the moonPhoebe at 19:33 UT inSpacecraft Event Time at 2068 kilometers distance. All of the eleven onboard instruments operated as expected and all data was acquired. Scientists plan to use the data to create global maps of the cratered moon, and to determine Phoebe's composition, mass and density. It took scientists several days to pore over the data to make more concrete conclusions.

16 June 2004 – TCM-21 took place with a 38-second main engine burn. It was planned as the last correction of the trajectory ofCassini before SOI. A few days later the final TCM-22 tentatively scheduled for 21 June was canceled.

1 July 2004 – The Saturn Orbit Insertion burn was successfully executed. At 7:11 p.m. PDT (10:11 p.m. EDT),Cassini crossed the ring plane between Saturn's F and G rings. Its antenna was oriented forward acting as a shield against small ring particles. At 7:36 p.m. PDT (10:36 p.m. EDT), the spacecraft began a critical 96-minute main engine burn to cut its velocity by 626 meters per second and permit a 0.02 x 9 million kilometer Saturn orbit. Right after that burn, pictures of the rings were taken and sent back to mission scientist as the spacecraft approached within 19,980 kilometers (12,400 miles) from the cloud tops.^[21] Scientists were surprised by the clarity and detail of the pictures and will be poring over them for quite some time. "We won't see the whole puzzle, only pieces, but what we are seeing is dramatic," said Dr.Carolyn Porco,Cassini imaging team leader, Space Science Institute, Boulder, Colo. "The images are mind-boggling, just mind-boggling. I've been working on this mission for 14 years and I shouldn't be surprised, but it is remarkable how startling it is to see these images for the first time."

2 July 2004 –Cassini's first flyby ofTitan was executed and first close up pictures were sent back to Earth. Due to the planning of the initial orbit,Cassini was passing over the south pole of the moon and from a larger distance than in later flybys. Regardless, during a press conference on 3 June,^{[clarification needed]} mission scientists presented pictures that were already causing them to rethink previous theories. It now seems that the darker and brighter albedo features on the surface do represent different materials. But in contrast to expectation, the icy regions seem to be darker than the areas where other (possibly organic) matter is mixed in with the ice.

16 August 2004 – Mission scientists announce the discovery of two new moons of Saturn, and with it the successful start of one of the programs ofCassini: Locating small and yet unknown moons. Later named "Methone" (S/2004 S 1) and "Pallene" (S/2004 S 2), these objects are small compared to other moons and they orbit betweenMimas andEnceladus.

23 August 2004 – At a distance of 9 million kilometers from Saturn, the last major firing of the main engine took place to adjust the next closest approach and avoid the particles in the ring system. The 51 minute burn increased the velocity of the probe by 325 meters per second, moving the orbitalperiapsis point about 300,000 km farther away from Saturn than its smallest distance during SOI. At the same time, the new course will bringCassini very close to Titan on its next flyby.^[22]

14 September 2004 – Final checks of theHuygens lander were completed successfully.

26 October 2004 – The second flyby of Titan (called "Titan-A") was successfully executed. Data started to arrive at the JPL mission center at 01:30 UTC, 27 October, and included the highest resolution pictures ever taken of the surface of that moon. Additionally, first high-resolution infra-red spectra and pictures were taken from the atmosphere and surface. The spacecraft successfully skimmed the hazy, smoggy atmosphere of Titan, coming within 1,176 kilometers of Titan's surface. The flyby was the closest that any spacecraft has ever come to Titan. The pictures, spectra, and radar data revealed a complex, puzzling surface. The only glitch during the "Titan-A" event involved the CIRS instrument. During playback, the instrument team observed corrupted data. A decision was made to power the instrument off to reboot it. CIRS was powered back on within 24 hours and returned to its nominal state.

23 November 2004 – The last in-flight checks of theHuygens probe before separation were completed successfully.

13 December 2004 – The "Titan-B" flyby was executed successfully.

25 December 2004 –Huygens probe separated fromCassini orbiter at 02:00 UTC.^[23]

27 December – NASA published a picture ofHuygens taken fromCassini two days after its release. It reported that the analysis of that picture shows that the probe is on the correct course within the expected error range. These checks were necessary in order to placeCassini in the correct orientation to receive the data fromHuygens when it entered Titan's atmosphere.

28 December 2004 – OTM-10 was executed at 03:00UTC inSpacecraft Event Time. This maneuver, also called the Orbit Deflection Maneuver (ODM), tookCassini off of a Titan-impacting trajectory and on to a flyby trajectory with the required altitude to receive data from theHuygens probe as it plunged into Titan's thick atmosphere.

31 December 2004 –Cassini's flyby of Iapetus occurred at 18:45:37 UTC at an altitude of 122645 kilometers. First raw pictures were available the next day.

14 January 2005 –Huygens entered Titan's atmosphere at 09:06 UTC and landed softly on its surface about two hours later. This was confirmed by the reception of thecarrier wave emitted by the probe during its descent and touchdown. At 16:19 UTC, theCassini orbiter started to relay the scientific data received from the probe to Earth. The first picture was released at 19:45 UTC, showing a view from about 16 km above the surface. A second picture taken from the probe at rest on the surface was released a short time later.

15 February 2005 –Cassini executed a successful Titan flyby, with new regions of its surface scanned byradar.Cassini's mapping radar acquired a picture that shows a largecrater on Titan, with an estimated diameter of 440 km (270 mi).^[24]

17 February 2005 – The first close flyby ofEnceladus was executed and the first closeup images were sent back to Earth. The flyby distance was about 1,180 km (730 mi).

17 March 2005 – TheCassini probe revealed that Saturn's moon Enceladus has an atmosphere. It has been described as "substantial" by its discoverers.

16 April 2005 – The fifth planned flyby of Titan with a minimum distance of about 1,025 kilometers was executed at 19:12 UTC. This was the closest flyby up to this date, and provided the opportunity to obtain more detailed data on the constituents in the upper atmosphere of Titan. The first analysis of that data showed a large range of complex carbonmolecules. On 25 April a mass plot was published that demonstrates the existence of these molecules.

3 May 2005 –Cassini beginsRadio occultation experiments onSaturn's Rings, to determine ring particle size distribution, on the scale of centimeters.

10 May 2005 – At the beginning of a period of focussed observation of the ring system of Saturn, slated to take until September, mission scientists announced the discovery of a new moon in the "Keeler gap" inside the "A" ring. Provisionally named S/2005 S 1 and later namedDaphnis, it was first seen in a time-lapse sequence of images taken on 1 May. Imaging scientists had predicted the new moon's presence and its orbital distance from Saturn after last July's sighting of a set of peculiar spiky and wispy features in the Keeler gap's outer edge.

14 July 2005 – The closest flyby of Enceladus with a distance of 175 km (109 mi) was executed successfully. First raw pictures were published.

7 September 2005 – Flyby of Titan at a distance of 1,075 km (668 mi), data gathered partially lost due to software problem.

26 September 2005 – Flyby ofHyperion at a distance of 1,010 km (630 mi), the closest flyby and only visit to the moon during the primary mission.

27 July 2006 – NASA confirms the presence of hydrocarbon lakes in Titan's northern polar region.

28 May 2008 –Cassini completed its 43rd flyby of Titan, ending its primary mission. RenamedCassini Equinox mission,Cassini observed Saturn during its equinox crossing, or summertime.^[25]

9 August, 11 August, 9 October, and 31 October 2008 – With closest approach at 50, 25, and 200 km, respectively,Cassini's last three Enceladus flybys of 2008 utilized a new imaging technique named "skeet shooting" to successfully acquire very high resolution images. Theflybys also allowedCassini to directly sample Enceladus'scryovolcanic plumes.

3 November, 14 November, 5 December, and 21 December 2009 – Titan flybys 46 through 49 concentrated on radar, VIMS, and INMS sampling of Titan and its thick atmosphere. T47 involved high-resolution VIMS coverage of the Huygens landing site, while the other three flybys made use of radar and RSS. T49 allowed radar coverage of Ontario Lacus, one of the largest methane lakes on Titan.

June - October 2009 –Cassini observed Saturn during its equinox, or the time of Saturn's year where the sun is directly over its equator.^[26]

2 November 2010 –Cassini was triggered into a protective standby mode, or "safe mode", after a bit flip caused it to miss an important instruction. NASA announced the interruption in scientific processes on 8 November.^[27] However, by 8 November some of the craft's functionality had already been partly restored.^[28] Nominal scientific instrument sequencing events were successfully started on 10 November.^[29][30]Cassini was reactivated as scheduled on 24 November and has returned to perfect working order, in time for two scheduled close fly-bys withEnceladus.^[31] At this point there has been no public disclosure^[32] as to the data loss impact of the 11 November (T-73) flyby. However, no images were acquired on the 11 November polar flyby.

On 3 February 2010, NASA announced that a second mission extension until May 2017, a few months past Saturn'ssummer solstice, had been funded. The schedule included an additional 155 orbits, with 54 flybys of Titan, 11 of Enceladus,^[33] 2 of Rhea, and 3 of Dione. One of the flybys of Titan dipped below the ionosphere.

On 15 September 2017,Cassini was deliberately disposed of by a controlled fall intoSaturn's atmosphere, ending its nearly two-decade-long mission.^[2][34] The last signal was received at 11:55:46 UTC.

This section needs to beupdated. Please help update this article to reflect recent events or newly available information.(September 2017)

All times given after 2005-Jan-14 09:11 UTC are expected event times and may differ from actual event times. This page will be updated after descent has occurred with corrections if they are necessary.^{[needs update][36][37]}

The data used in this section has been slightlyout of date, an updated version of ephemeris from ESA was available 2005 January 6.^{[citation needed]}

Following is a list of close fly-bys of Saturn's moons (at less than 5000 km). The closest approach for each moon is bolded.

The second extended mission was scheduled from 2010 October 12 through the Saturnian summer solstice in May 2017, followed by two dozen proximal orbits of Saturn and the rings.Cassini's final optical navigation image of the mission was taken on 20 September 2016.^[38] TheCassini mission ended on 15 September 2017, when the craft disintegrated in Saturn's atmosphere.^[34]

Proximal orbits

• Cassini–Huygens press release archives
• "Cassini–Huygens Saturn Arrival" June 2004 (pdf)
• Draft White paper for Solar System Decadal Survey 2013–2023: Cassini–Huygens Solstice Mission 2009 (pdf)
• Tour dates

• Cassini–Huygens
• Spaceflight timelines

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