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Rosetta Mission
“Great Comet of 1577”
השביטים נמצאים בשני אזורים עיקריים: 
עננת אורט: לא ניתן לצפות בה ישירות בגלל המרחק ) 100 -50 אלף 
יחידות אסטרונומיות( וגם בגלל שהשביטים אינם מאירים באזור זה. 
משערים כי מקור השביטים באזור זה הוא מכוכבי הלכת הגדולים של 
מערכת השמש. 
שביטים עוזבים את העננה כתוצאה מהשפעת כוח כבידה של כוכבים 
החולפים באזור. הערכה היא שכל שנה נכנסים כ 10 - שביטים לתוך 
מערכת השמש. שביטים אלו הם בעלי זמן מחזור ארוך. 
חגורת קויפר: שביטים בעלי מחזור קצר ) קטן מ 200 - שנה ( מגיעים 
מחגורת קויפר הממוקמת במרחק של 60 -30 יחידות אסטרונומיות
ROSETTA EQM
This photo shows Rosetta being tested before it was wrapped in 
insulating blankets and loaded on a rocket for launch.
Rosetta has massive solar wings to power the 
spacecraft. They were unfurled and checked out at the 
European Space Agency's test facilities before being 
packed up for liftoff.
Rosetta's mission started on March 2, 2004, 
when it was launched on a European Ariane 5 
rocket from Kourou, French Guiana.
Deep space manoeuvres 
• To achieve the required velocity to rendezvous with 
67P/C-G, Rosetta used gravity assist manoeuvres to 
accelerate throughout the Inner solar system
February 2007 
Rosetta took this image of Mars as it 
looped through the solar system
ROSETTA’S SELF-PORTRAIT 
AT MARS 
25th February 2007
November 2007 
After its closest approach to Earth Rosetta 
captured this image of the planet.
Rosetta passed asteroid 2867 Šteins in, giving scientists 
amazing close-ups of the asteroid's huge crater. The 
asteroid is about 3 miles in diameter. 
September 2008
November 2009 
Rosetta snapped this image of Earth in November 2009. 
The spacecraft was 393,328 miles from Earth.
Beautiful Lutetia 
10 July 2010 
• Flew by and photographed the asteroid 21 
Lutetia.
Lutetia and Saturn in the Background
Go to sleep Rosetta! 
8 June 2011 
• The spacecraft was transferred into a spin 
stabilised mode and all electronics except the 
on-board computer and the hibernation 
heaters were switched off
Three and a Half years 
Later…..
Wake-Up Rosetta! 
20 January 2014 
• At 10:00 UTC the spacecraft computer was 
taken out of hibernation mode and started 
post-hibernation procedures. 
• Rosetta restored communications with ESOC 
through NASA's Goldstone ground station at 
18:18 UTC
https://www.youtube.com/watch?v=tr 
ljrwTbr4w
Wake-Up Rosetta!
March 2014 
ROSETTA’S FIRST SIGHTING OF ITS TARGET
April 2014
June 2014 
67P/Churyumov–Gerasimenko
June 2014 
FIRST DETECTION OF WATER VAPOUR
14th of July 2014 picture 
14th July 2014
A model of the comet's shape, based 
on the images acquired on 14 July 201
the nucleus of comet 67P/Churyumov- 
Gerasimernko from a distance of 1,210 miles 
(1,950 kilometers).. 
29 July2014
2 August 2014 
Comet activity on 2 August 2014
3 August 2014 
Comet 67P/Churyumov-Gerasimenko by Rosetta’s OSIRIS narrow-angle camera on 3 August from 
a distance of 285 km. The image resolution is 5.3 metres/pixel.
Arrive to the Comet! 
7 minutes of maneuver. 
6 August 2014
Comet 67P/Churyumov-Gerasimenko by Rosetta’s OSIRIS narrow-angle camera on 3 August from 
a distance of 285 km. The image resolution is 5.3 metres/pixel.
Stunning close up detail focusing on a smooth region on the ‘base’ of the ‘body’ section of 
comet 67P/Churyumov-Gerasimenko. The image was taken by Rosetta’s OSIRIS narrow-angle 
camera and downloaded today, 6 August. The image clearly shows a range of features, including 
boulders, craters and steep cliffs. 
The image was taken from a distance of 130 km and the image resolution is 2.4 metres per 
pixel.
.
In Orbit around 67P/C-G! 
• In August 2014, Rosetta rendezvoused with the comet, 
commencing an approach to it on a triangular path 
whose segments are hyperbolic escape trajectories, 
alternating with thruster burns. 
• After closing to within about 30 km (19 mi) from the 
comet the spacecraft will enter actual orbit about 
it,[7][8] in preparation for releasing a lander that will 
make contact with the comet itself. 
• The exact surface layout of the comet is currently 
unknown and the orbiter has been built to map this 
before detaching the lander. It is anticipated that a 
suitable landing site can be found, although few 
specific details exist regarding the surface
ROSETTA'S COMET IN 3D
20 August 2014 
Rosetta navigation camera image taken on 20 
August 2014 at about 83 km from comet 
67P/Churyumov-Gerasimenko. The comet 
nucleus is about 4 km across.
21 August 2014
24 August 2014 
FROM FAR VS VERY CLOSE
25 August 2014 
PHILAE CANDIDATE LANDING SITES
CANDIDATE LANDING SITE A
CANDIDATE LANDING SITE B
CANDIDATE LANDING SITE J
5 September 2014 
COMET ON 5 SEPTEMBER 2014
19 September 2014
ROSETTA COMET OBSERVED WITH VERY LARGE TELESCOPE 
8 m-diameter telescopes of the European Southern Observatory’s Very Large Telescope in Chile.
2 October 2014
15 October 2014 
Philae’s primary landing site
Delivering Philae to Agilkia
Graphical timeline of the Philae landing
Time at spacecraft Time on Earth 
Event Time (rel) Time (SCET, UT) Time (CET) Time (UT) Time (PT) 
Rosetta Google Hangout -- -- Nov 7 16:00 Nov 7 15:00 Nov 7 07:00 
ESOC media update (ESA TV) -- -- Nov 10 15:00 Nov 10 14:00 Nov 10 06:00 
ESOC media update (ESA TV) -- -- Nov 11 11:00 Nov 11 10:00 Nov 11 02:00 
24-hour ESA #CometLanding Livestream begins -- -- Nov 11 20:00 Nov 11 19:00 Nov 11 11:00 
Go/no-go decision 1: proceed to downlink landing instructions to 
Philae 
-- -- Nov 11 20:35 Nov 11 19:35 Nov 11 11:35 
ESOC media update (ESA TV) -- -- Nov 11 20:30 Nov 11 19:30 Nov 11 11:30 
Go/no-go decision 2: ready for separation -- -- Nov 11 01:00 Nov 11 00:00 Nov 10 16:00 
Go/no-go decision 3: proceed for delivery maneuver -- -- Nov 12 02:35 Nov 12 01:35 Nov 11 17:35 
Rosetta pre-delivery maneuver (lining up for separation) -2h Nov 12 06:35 Nov 12 08:03 Nov 12 07:03 Nov 11 23:03 
ESOC media update (ESA TV) -- -- Nov 12 07:15 Nov 12 06:15 Nov 11 22:15 
Go/no-go decision 4: proceed for landing -- -- Nov 12 08:35 Nov 12 07:35 Nov 11 23:35 
Lander separation (22.5 km from comet); Separation, Descent, 
and Landing phase begins 
+0h Nov 12 08:35 Nov 12 10:03 Nov 12 09:03 Nov 12 01:03 
Rosetta divert maneuver +40m Nov 12 09:15 Nov 12 10:43 Nov 12 09:43 Nov 12 01:43 
ESOC receives CIVA "farewell" image -- -- Nov 12 11:00 Nov 12 10:00 Nov 12 02:00 
Rosetta point to Philae +2h Nov 12 10:35 Nov 12 12:03 Nov 12 11:03 Nov 12 03:03 
Possible release of NavCam and/or CIVA "farewell" images -- -- Nov 12 13:00 Nov 12 12:00 Nov 12 04:00 
Landing (time approx) +7h Nov 12 15:35 Nov 12 17:03 Nov 12 16:03 Nov 12 08:03 
ESOC receives CIVA panorama -- -- Nov 12 17:35 Nov 12 16:35 Nov 12 08:35 
Possible presentation of first images -- -- Nov 12 18:00 Nov 12 17:00 Nov 12 09:00 
First science sequence begins Landing +1h Nov 12 16:35 Nov 12 18:03 Nov 12 17:03 Nov 12 09:03 
24-hour ESA #CometLanding Livestream ends -- -- Nov 12 19:00 Nov 12 18:00 Nov 12 10:00 
ESOC media update (ESA TV) -- -- Nov 13 14:00 Nov 13 13:00 Nov 13 05:00 
First science sequence ends Landing +65h Nov 15 08:35 Nov 15 10:03 Nov 15 09:03 Nov 15 01:03
PHILAE’S INSTRUMENTS
Philae lander 
November 2014 
• The lander, named Philae, will approach Churyumov– 
Gerasimenko at relative speed around 1 m/s (2.2 mph; 
3.6 km/h) and on contact with the surface, 
two harpoons will be fired into the comet to prevent the 
lander from bouncing off. 
• Additional drills are used to further secure the lander on 
the comet. 
• After its attachment to the comet, expected to take place in 
November 2014, the lander will begin its science mission: 
– Characterisation of the nucleus 
– Determination of the chemical compounds present, 
including enantiomers[34] 
– Study of comet activities and developments over time
bibliography 
http://rosetta.jpl.nasa.gov/gallery/images/co • 
met-67p/churyumov-gerasimenko 
https://en.wikipedia.org/wiki/Rosetta_(spacec • 
raft) 
http://www.esa.int/spaceinimages/content/se • 
arch?SearchText=rosetta&img=1&SearchButto 
n=Go
• http://rosetta.esa.int/ 
• http://rosetta.jpl.nasa.gov/

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Rosetta mission

  • 2.
  • 4.
  • 5. השביטים נמצאים בשני אזורים עיקריים: עננת אורט: לא ניתן לצפות בה ישירות בגלל המרחק ) 100 -50 אלף יחידות אסטרונומיות( וגם בגלל שהשביטים אינם מאירים באזור זה. משערים כי מקור השביטים באזור זה הוא מכוכבי הלכת הגדולים של מערכת השמש. שביטים עוזבים את העננה כתוצאה מהשפעת כוח כבידה של כוכבים החולפים באזור. הערכה היא שכל שנה נכנסים כ 10 - שביטים לתוך מערכת השמש. שביטים אלו הם בעלי זמן מחזור ארוך. חגורת קויפר: שביטים בעלי מחזור קצר ) קטן מ 200 - שנה ( מגיעים מחגורת קויפר הממוקמת במרחק של 60 -30 יחידות אסטרונומיות
  • 6.
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  • 14.
  • 15. This photo shows Rosetta being tested before it was wrapped in insulating blankets and loaded on a rocket for launch.
  • 16. Rosetta has massive solar wings to power the spacecraft. They were unfurled and checked out at the European Space Agency's test facilities before being packed up for liftoff.
  • 17.
  • 18. Rosetta's mission started on March 2, 2004, when it was launched on a European Ariane 5 rocket from Kourou, French Guiana.
  • 19.
  • 20.
  • 21.
  • 22. Deep space manoeuvres • To achieve the required velocity to rendezvous with 67P/C-G, Rosetta used gravity assist manoeuvres to accelerate throughout the Inner solar system
  • 23.
  • 24. February 2007 Rosetta took this image of Mars as it looped through the solar system
  • 25. ROSETTA’S SELF-PORTRAIT AT MARS 25th February 2007
  • 26. November 2007 After its closest approach to Earth Rosetta captured this image of the planet.
  • 27.
  • 28. Rosetta passed asteroid 2867 Šteins in, giving scientists amazing close-ups of the asteroid's huge crater. The asteroid is about 3 miles in diameter. September 2008
  • 29. November 2009 Rosetta snapped this image of Earth in November 2009. The spacecraft was 393,328 miles from Earth.
  • 30. Beautiful Lutetia 10 July 2010 • Flew by and photographed the asteroid 21 Lutetia.
  • 31.
  • 32. Lutetia and Saturn in the Background
  • 33. Go to sleep Rosetta! 8 June 2011 • The spacecraft was transferred into a spin stabilised mode and all electronics except the on-board computer and the hibernation heaters were switched off
  • 34. Three and a Half years Later…..
  • 35. Wake-Up Rosetta! 20 January 2014 • At 10:00 UTC the spacecraft computer was taken out of hibernation mode and started post-hibernation procedures. • Rosetta restored communications with ESOC through NASA's Goldstone ground station at 18:18 UTC
  • 38. March 2014 ROSETTA’S FIRST SIGHTING OF ITS TARGET
  • 41. June 2014 FIRST DETECTION OF WATER VAPOUR
  • 42. 14th of July 2014 picture 14th July 2014
  • 43.
  • 44.
  • 45.
  • 46. A model of the comet's shape, based on the images acquired on 14 July 201
  • 47. the nucleus of comet 67P/Churyumov- Gerasimernko from a distance of 1,210 miles (1,950 kilometers).. 29 July2014
  • 48. 2 August 2014 Comet activity on 2 August 2014
  • 49. 3 August 2014 Comet 67P/Churyumov-Gerasimenko by Rosetta’s OSIRIS narrow-angle camera on 3 August from a distance of 285 km. The image resolution is 5.3 metres/pixel.
  • 50.
  • 51.
  • 52. Arrive to the Comet! 7 minutes of maneuver. 6 August 2014
  • 53.
  • 54. Comet 67P/Churyumov-Gerasimenko by Rosetta’s OSIRIS narrow-angle camera on 3 August from a distance of 285 km. The image resolution is 5.3 metres/pixel.
  • 55. Stunning close up detail focusing on a smooth region on the ‘base’ of the ‘body’ section of comet 67P/Churyumov-Gerasimenko. The image was taken by Rosetta’s OSIRIS narrow-angle camera and downloaded today, 6 August. The image clearly shows a range of features, including boulders, craters and steep cliffs. The image was taken from a distance of 130 km and the image resolution is 2.4 metres per pixel.
  • 56.
  • 57.
  • 58. .
  • 59.
  • 60. In Orbit around 67P/C-G! • In August 2014, Rosetta rendezvoused with the comet, commencing an approach to it on a triangular path whose segments are hyperbolic escape trajectories, alternating with thruster burns. • After closing to within about 30 km (19 mi) from the comet the spacecraft will enter actual orbit about it,[7][8] in preparation for releasing a lander that will make contact with the comet itself. • The exact surface layout of the comet is currently unknown and the orbiter has been built to map this before detaching the lander. It is anticipated that a suitable landing site can be found, although few specific details exist regarding the surface
  • 62. 20 August 2014 Rosetta navigation camera image taken on 20 August 2014 at about 83 km from comet 67P/Churyumov-Gerasimenko. The comet nucleus is about 4 km across.
  • 64. 24 August 2014 FROM FAR VS VERY CLOSE
  • 65.
  • 66. 25 August 2014 PHILAE CANDIDATE LANDING SITES
  • 70. 5 September 2014 COMET ON 5 SEPTEMBER 2014
  • 72. ROSETTA COMET OBSERVED WITH VERY LARGE TELESCOPE 8 m-diameter telescopes of the European Southern Observatory’s Very Large Telescope in Chile.
  • 74.
  • 75. 15 October 2014 Philae’s primary landing site
  • 76.
  • 77.
  • 79. Graphical timeline of the Philae landing
  • 80. Time at spacecraft Time on Earth Event Time (rel) Time (SCET, UT) Time (CET) Time (UT) Time (PT) Rosetta Google Hangout -- -- Nov 7 16:00 Nov 7 15:00 Nov 7 07:00 ESOC media update (ESA TV) -- -- Nov 10 15:00 Nov 10 14:00 Nov 10 06:00 ESOC media update (ESA TV) -- -- Nov 11 11:00 Nov 11 10:00 Nov 11 02:00 24-hour ESA #CometLanding Livestream begins -- -- Nov 11 20:00 Nov 11 19:00 Nov 11 11:00 Go/no-go decision 1: proceed to downlink landing instructions to Philae -- -- Nov 11 20:35 Nov 11 19:35 Nov 11 11:35 ESOC media update (ESA TV) -- -- Nov 11 20:30 Nov 11 19:30 Nov 11 11:30 Go/no-go decision 2: ready for separation -- -- Nov 11 01:00 Nov 11 00:00 Nov 10 16:00 Go/no-go decision 3: proceed for delivery maneuver -- -- Nov 12 02:35 Nov 12 01:35 Nov 11 17:35 Rosetta pre-delivery maneuver (lining up for separation) -2h Nov 12 06:35 Nov 12 08:03 Nov 12 07:03 Nov 11 23:03 ESOC media update (ESA TV) -- -- Nov 12 07:15 Nov 12 06:15 Nov 11 22:15 Go/no-go decision 4: proceed for landing -- -- Nov 12 08:35 Nov 12 07:35 Nov 11 23:35 Lander separation (22.5 km from comet); Separation, Descent, and Landing phase begins +0h Nov 12 08:35 Nov 12 10:03 Nov 12 09:03 Nov 12 01:03 Rosetta divert maneuver +40m Nov 12 09:15 Nov 12 10:43 Nov 12 09:43 Nov 12 01:43 ESOC receives CIVA "farewell" image -- -- Nov 12 11:00 Nov 12 10:00 Nov 12 02:00 Rosetta point to Philae +2h Nov 12 10:35 Nov 12 12:03 Nov 12 11:03 Nov 12 03:03 Possible release of NavCam and/or CIVA "farewell" images -- -- Nov 12 13:00 Nov 12 12:00 Nov 12 04:00 Landing (time approx) +7h Nov 12 15:35 Nov 12 17:03 Nov 12 16:03 Nov 12 08:03 ESOC receives CIVA panorama -- -- Nov 12 17:35 Nov 12 16:35 Nov 12 08:35 Possible presentation of first images -- -- Nov 12 18:00 Nov 12 17:00 Nov 12 09:00 First science sequence begins Landing +1h Nov 12 16:35 Nov 12 18:03 Nov 12 17:03 Nov 12 09:03 24-hour ESA #CometLanding Livestream ends -- -- Nov 12 19:00 Nov 12 18:00 Nov 12 10:00 ESOC media update (ESA TV) -- -- Nov 13 14:00 Nov 13 13:00 Nov 13 05:00 First science sequence ends Landing +65h Nov 15 08:35 Nov 15 10:03 Nov 15 09:03 Nov 15 01:03
  • 81.
  • 83. Philae lander November 2014 • The lander, named Philae, will approach Churyumov– Gerasimenko at relative speed around 1 m/s (2.2 mph; 3.6 km/h) and on contact with the surface, two harpoons will be fired into the comet to prevent the lander from bouncing off. • Additional drills are used to further secure the lander on the comet. • After its attachment to the comet, expected to take place in November 2014, the lander will begin its science mission: – Characterisation of the nucleus – Determination of the chemical compounds present, including enantiomers[34] – Study of comet activities and developments over time
  • 84.
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  • 91.
  • 92. bibliography http://rosetta.jpl.nasa.gov/gallery/images/co • met-67p/churyumov-gerasimenko https://en.wikipedia.org/wiki/Rosetta_(spacec • raft) http://www.esa.int/spaceinimages/content/se • arch?SearchText=rosetta&img=1&SearchButto n=Go
  • 93. • http://rosetta.esa.int/ • http://rosetta.jpl.nasa.gov/