prisma_logotype_sve
About PrismaMission eventsNewsOrganisationContactsIMAGES
Tango Separation

(Duration of 5 days)


The Tango spacecraft will be separated from Mango in a direction such that the relative orbit will be safe even without active thrusting. The separation will also allow for good viewing conditions with the VBS and DVS.

The orbit control functionality on Mango will be disabled during the first orbits after separation. After evaluation of the separation impulse, a ground calculated cancellation delta-V will be executed to keep the two satellites close to each other in near future. After additional assessment of the GPS navigation and orbit control functions, the autonomous orbit control will be enabled.

Reports:

Separation anxiety

As any mother when their offspring eventually leave the nest, Mango felt a tinge of cold feet and aloneness when Tango separated and left on her journey in to dark space.  This was seen as an expected sinking of temperatures on Mango right after Tango was let go.  Some of Mango's components are plotted below...

Mango sep temperatures

Tango, out on her own now in the cold black space, felt much the same and her temperatures dropped as well upon leaving Mango.  Some of Tango's hardware temperatures are plotted below...

Tango sep temperatures

The more rational engineering explanation is that while mated, there were large radiators on both Mango and Tango that were blocked by each other (on the surface areas that were between the two spacecraft), and hence these radiators did not have much cooling effect as their "view" to cold space was poor.  Upon separation, these radiator surfaces were opened up, exposing both the Mango and Tango radiators to cold space, hence cooling the spacecraft down considerably.  This was anticipated and both Mango and Tango responded accordingly by turning on internal heaters to regulate their temperatures.  Now, a number of days later, they are happy and warm flying together through space! 

Written by 
Nils Pokrupa
 
2010-08-17 / 04:20:52

TANGO Final Commissioning: Reference Attitude Profile tracking

After a smooth Sun Acquisition on Wednesday, some calibration process on Thursday and a successful transition to Sun Zenith pointing mode yesterday, the final commissioning tests have been performed on TANGO today. The goal was to push the spacecraft magnetic control towards its limits. Indeed, we forced TANGO to follow different attitude profiles that were extreme cases for TANGO:

-         attitudes that are normally instable points with respect to Gravity Gradient

-         rotation axis “far away” from the orbit normal

-         sun on the edge (and sometimes exiting) the fine Sun Sensor field of view

But TANGO worked hard and successfully managed to follow the profiles, within the required +/-25 deg expected accuracy.

TANGO is now fully commissioned and ready for the rest of the mission.

TARGET_referenceTrackingProfile_1

Written by 
Camille Chasset
 
2010-08-15 / 08:21:26

TANGO converged to Sun Zenith Pointing Mode

Yesterday, TANGO successfully performed a transition to Sun Zenith pointing mode. As TANGO is only controlled by Magnetotorquers (like electro-magnets interacting with the Earth magnetic field) it has to be handled with extra care, and all manoeuvres require time and patience. To give you an idea, the typical time constant for any attitude manoeuvre on TANGO is in the order of a few hours.

So TANGO slowly reduced its initial Safe Mode rate (about 0.5 deg/s) and accomplished its manoeuvre to enter its nominal working mode: Sun / Zenith. This means that it points its Solar Array towards the Sun, and its GPS antenna towards Zenith.

The manoeuvre as well as the steady state reached by TANGO afterwards were as expected.

TANGO_sun_zenith_transition_1

Written by 
Camille Chasset
 
2010-08-15 / 07:56:23

TLEs

Mango and Tango are now in the NORAD Two Line Element (TLE) database. Mango has the SSC number 36599 (same as the combined Prisma) and Tango has the SSC number 36827. So now all you who have a satellite viewer app on your phone or computer should update it with two satellites.

Currently the two TLEs, as defined by NORAD, are

PRISMA (MANGO)
1 36599U 10028B   10226.72746116 -.00000722  00000-0 -20967-3 0  1989
2 36599 098.2816 051.9974 0043696 014.2636 345.9769 14.40867728  8652

PRISMA (TANGO)
1 36827U 10028F   10226.72746162 -.00000393  00000-0 -10830-3 0   110
2 36827 098.2805 051.9964 0043468 014.1714 346.0686 14.40868278   413

Written by 
Erik Clacey
 
2010-08-15 / 01:23:29

Tango posing for the camera

DVS_0856_Image_00010_mini

DVS_0856_Image_00010.jpg

As Tango is making its way towards Sun Zenith pointing we took the opportunity to also test one of the attitude pointing modes of Mango: GPS based pointing towards Tango. This mode will eventually be used by several of the experiments, among them both FFRF and VBS. As the telemetry showed us that the attitude manoeuvre was complete we took the opportunity to take some new images with the DVS camera. The result was a stunning image of Tango flying solo, about 100 meters away. Zooming in you can clearly make out details such as the FFRF and ISL antennas.

Written by 
Niklas Ahlgren
 
2010-08-14 / 04:01:14

Everything nominal

Tonight we have been busy with checkout of Tango and first analyses of the relative dynamics for the satellite constellation Mango & Tango. A few updates of estimation control parameters have been identified and updated on-board. This was according to plans and in general everything is going very smooth.

The drift cancelation delta-V that was performed yesterday was judged successful enough such that a correction delta-V was unnecessary. The correction delta-V was scheduled a few orbits later in the separation sequence that Ron posted on the blog.

Since the cancelation delta-V Mango has been left to slowly drift closer to Tango again. During this time we are collecting data of the natural relative orbit dynamics between the two spacecrafts. Even though it looks like they will soon come very close in the figure, the relative orbit is completely safe. The closest encounter during the next days is estimated to be a minimum of 35 meters if Mango is left on a free drift trajectory.

PRISMA_separation_relative_orbit_1_5_days

As you might notice in the figure, we are still tuning the GPS navigation, some small jumps are still visible.

Written by 
Robin Larsson
 
2010-08-13 / 09:24:37

Relative GPS Navigation

As Prisma entered this new phase of the mission the operations team have to deal with some new challenges. There are now two spacecrafts to monitor and control, and as they are very close to each other it becomes crucial to have a good knowledge about the relative position between them at all times. The system has of course been designed with this in mind. Almost all functions can be handled autonomously on-board, but all this is experimental and needs a careful examination in-orbit and that the complexity is increased in steps.

One key function is the GPS navigation, for Prisma this function is developed by DLR and then integrated into the on-board software by SSC. The function provides precise position and velocity for both spacecrafts at any time, necessary to determined if a maneuver is needed to maintain the constellation.

The separation event is a challenging task for the GPS navigation as it is the only time in the mission where an impulse will be applied to Tango. The preliminary analysis done during the night has shown a nominal and well behaved GPS navigation. The accuracy is expected to be very good almost directly after the separation. As you can see in the figure below the motion is smooth with only a few jumps, these are related to periods where the GPS receivers where off as Mango was flying through the south Atlantic anomaly.

PRISMA_TargetSeparation_relative_orbit

Figure showing the relative motion before and after the separation event. In these plots Tango is fixed at [0 0] and the relative motion done by Mango is drawn out. Tango's location is shown with a "+" and the last position of Mango is shown with a "o".

The three dimensional relative motion is shown from three different sides, the first plot is looking at the motion from above, second one from the side (cross-track) and the third one from the direction where both satellites are flying (along-track). The last plot shows the relative motion on a timescale. All lines start close together, before separation, and then drift apart until the drift cancelation maneuver is performed around midnight.

Written by 
Robin Larsson
 
2010-08-12 / 09:18:41

Tango's first sun acquisition

Tonight was a special night also for the smaller one of the two Prisma satellites. Tango has since launch been very passive, sitting clamped to Mango which has done all the control. Tonight Tango took a leap out in space, controlling it's own attitude directly after separation. Using only magnetorquers to create a momentum that turns the satellite in the correct direction. For the first days Tango points it's solar array towards the sun and rotates slowly around the sun vector. Later the rotation will be stopped and the attitude 3-axis stabilized.

 

This video is focusing on Tango at the separation event. After separation the slowly tumbling Tango is quickly estimating the sun direction and creates the correct momentum to acquire the sun.

Written by 
Robin Larsson
 
2010-08-12 / 07:41:29

Satellite Formation Flying!

Tonight has been a very special night. The Prisma satellites has been developed, built and tested with the primary objective to demonstrate satellite formation flying. This night we have started to demonstrate satellite formation flying. Two small spacecrafts orbiting earth with a speed of 7km/s, maintained in a constellation controlled at meter level.

 

Have a look at this video showing the separation event and also a little later the first maneuver performed by Mango to cancel the drift away from Tango. This is the first small step to enable an actively controlled satellite constellation. The video is generated from on-board navigation data.

 

 

Written by 
Robin Larsson
 
2010-08-12 / 06:43:27

Listen to the Intersatellite Link

Sven Grahn provided us with a snap shot from space: he picked up the signal from the radio link that connects Mango and Tango, the so called inter-satellite link or ISL. The ground station in Kiruna only listens to radio link of Mango, and the data from Tango is echoed by Mango over that link. But Mango and Tango continuously chat over this ISL, and apparantly it is strong enough so that Sven can hear it in his back yard in Eskilstuna. You can listen to a short sample here. It was recorded today august 11, approximately 1820 UTC. The signal is slowly rising in pitch, which is the Doppler effect, as the satellite flies over Sweden.

 


Written by 
Ron Noteborn
 
2010-08-12 / 00:10:00

First in-orbit image of Tango

 

 Target Separated

We followed the entire separation from Mango with the video camera developed by TechnoSystems and got the first few images down to ground during the first passage after separation. Fully lit by the sun against the blackness of space we can still clearly make out the FFRF antennas and can that the separation worked flawlessly. We will continue to download more images throughout the night, so we are hoping for further images of Tango starting its own journey in space.

 

All systems look to be working as expected, sun pointing was achieved very quickly so the battery aboard Tango was rapidly starting charging and the platform looks very stable.

Written by 
Niklas Ahlgren
 
2010-08-11 / 21:33:41

Tango Separation Successful!

Passage 823 completed and we had all reason to open the champagne: telemetry indicated that Tango was free flying and had stabilised itself in a slowly rotating sun pointing attitude. Battery was nominal and solar array is working. Everything is fine aboard Tango. The GPS navigation shows that the relative trajectory is nominal: distance had increased to about 120m. The relative velocity at separation was at the right magnitude and the induced momentum was very good. Tango only had to remove a tumbling of about 1 deg/s. We are looking at the DVS images coming in and continue to follow the trajectory closely. Stay tuned for more news soon.
Written by 
Ron Noteborn
 
2010-08-11 / 21:08:17

Tango set for Separation

We just completed passage 822, in which we enabled the video system and released the command queues onboard. Battery on Target was shortly enabled for a final check, which was nominal. Just over an hour is left for separation. Everything is still looking green.
Written by 
Ron Noteborn
 
2010-08-11 / 18:51:23

Sequences Loaded

We completed the first passage of the day, and found Prisma in good health. All sequences were uploaded, and the command sequence to achieve the separation attitude is armed. So far everything is green.
Written by 
Ron Noteborn
 
2010-08-11 / 17:16:21

Tango Separation Sequence Starting Tonight

Tonight we will start the sequence for the separation of the Tango satellite. The sequence of events (in UTC time) is given below. We're all set for this exciting day!

Wednesday august 11, 2010

Orbit

UTC Time

Event

821

14:54:12

Passage 1 (8:33)

GNC Configuration for Separation

Entrance to Manual Mode

Loading of Separation Attitude to TTQ

Loading of GNC Pointing Sequence to TTQ

Loading of Cancellation Delta V to TTQ

Releasing Separation Attitude from TTQ

 

15:20:52

GPS OFF (SAA start 15:28:45)

 

15:40:52

GPS ON (SAA end 15:33:00)

822

16:32:53

Passage 2 (11:42)

Target Battery Check

Go Ahead for Target Separation

Target GPS Antenna switch load on TTQ

Release of Target Separation Sequence from TTQ

Release of Cancellation Delta V from TTQ

Enabling and Configuration of DVS

 

16:56:00

GPS OFF (SAA start 16:59:00)

 

17:16:00

GPS ON (SAA end 17:13:00)

 

T-900s =

17:36:45

Rotation to Separation Attitude (valid for 3 hours)

Switch Target GPS Antenna

 

T-120s

DVS TTQ sequence starts

Separation Sequence starts

 

T-80s

Disable PTCRTU toggling

 

T-70s

Force PTCRTU B

 

T-60s

DVS Reset

Activation Target Batteries

 

T-45s

Target on Internal Power

 

T-5s

DVS record start (2Hz)

 

T-2s

Target Separation Arm

 

17:51:45 = T

Target Separation

 

T+20s

Enable PTCRTU toggling

 

T+40s

DVS Record Stop

 

T+50s

DVS Record Start (1Hz)

 

T+60s

Start of Main Target Pointing Sequence

 

T+150s

DVS Record Stop

 

T+160s

DVS Record Start (0.1Hz)

823

18:11:53

Passage 3 (12:08)

Disable DVS

Confirmation of Target Separation

Attitude Check

Trajectory Check

Target Sun Acquisition Inspection

 

T+23m (18:14:45)

DVS Record Stop

 

T+24m (18:15:45)

DVS Disable

 

18:36:00

GPS OFF (SAA start 18:39:00)

 

18:56:00

GPS ON (SAA end 18:53:00)

824

19:50:46

Passage 4 (11:02)

Possible update of Cancellation Delta V

Switch on Target SMAE (attitude estimator)

 

20:16:00

GPS OFF (SAA start 20:19:00)

 

20:36:00

GPS ON (SAA end 20:33:00)

825

21:29:10

Passage 5 (9:40)

Possible update of Cancellation Delta V

Switch on Target automatic GPS Antenna switching

 

21:55:37

GPS OFF (SAA start 21:59:00)

 

22:15:37

GPS ON (SAA end 22:12:15)

826

23:06:43

Passage 6 (9:27)

Reconfiguration of GNC

Entrance to Safe/Celestial Mode

Along Track Evaluation

Enable Target SMAE in attitude loop

 

23:41:44

Cancellation Delta V

827

2010-08-12

00:43:46

Passage 7 (10:37)

828

02:21:23

Passage 8 (11:48)

Possible upload of Correction Delta V

829

04:00:55

Passage 9 (11:42)

Possible upload of Correction Delta V

 

05:09:07

GPS OFF (SAA start 05:12:15)

 

05:29:07

GPS ON (SAA end 05:26:00)

830

05:42:25

Passage 10 (09:09)


Written by 
Ron Noteborn
 
2010-08-11 / 16:06:35
Swedish National Space Board, tel +46 8 627 64 80 · SSC, tel +46 8 627 62 00