How to land on a comet
-
0:01 - 0:06I'd like to take you on the epic quest
of the Rosetta spacecraft. -
0:06 - 0:10To escort and land the probe on a comet,
-
0:10 - 0:13this has been my passion
for the past two years. -
0:13 - 0:15In order to do that,
-
0:15 - 0:18I need to explain to you something
about the origin of the solar system. -
0:18 - 0:20When we go back
four and a half billion years, -
0:20 - 0:22there was a cloud of gas and dust.
-
0:22 - 0:26In the center of this cloud,
our sun formed and ignited. -
0:26 - 0:32Along with that, what we now know
as planets, comets and asteroids formed. -
0:32 - 0:36What then happened, according to theory,
-
0:36 - 0:40is that when the Earth had cooled down
a bit after its formation, -
0:40 - 0:44comets massively impacted the Earth
and delivered water to Earth. -
0:45 - 0:50They probably also delivered
complex organic material to Earth, -
0:50 - 0:53and that may have bootstrapped
the emergence of life. -
0:53 - 0:56You can compare this to having
to solve a 250-piece puzzle -
0:56 - 1:00and not a 2,000-piece puzzle.
-
1:00 - 1:03Afterwards, the big planets
like Jupiter and Saturn, -
1:03 - 1:06they were not in their place
where they are now, -
1:06 - 1:08and they interacted gravitationally,
-
1:08 - 1:12and they swept the whole interior
of the solar system clean, -
1:12 - 1:13and what we now know as comets
-
1:13 - 1:16ended up in something
called the Kuiper Belt, -
1:16 - 1:19which is a belt of objects
beyond the orbit of Neptune. -
1:19 - 1:23And sometimes these objects
run into each other, -
1:23 - 1:26and they gravitationally deflect,
-
1:26 - 1:30and then the gravity of Jupiter
pulls them back into the solar system. -
1:30 - 1:34And they then become the comets
as we see them in the sky. -
1:34 - 1:37The important thing here to note
is that in the meantime, -
1:37 - 1:40the four and a half billion years,
-
1:40 - 1:43these comets have been sitting
on the outside of the solar system, -
1:43 - 1:44and haven't changed --
-
1:44 - 1:47deep, frozen versions of our solar system.
-
1:47 - 1:49In the sky, they look like this.
-
1:49 - 1:51We know them for their tails.
-
1:51 - 1:53There are actually two tails.
-
1:53 - 1:57One is a dust tail,
which is blown away by the solar wind. -
1:57 - 2:00The other one is an ion tail,
which is charged particles, -
2:00 - 2:03and they follow the magnetic field
in the solar system. -
2:03 - 2:04There's the coma,
-
2:04 - 2:07and then there is the nucleus,
which here is too small to see, -
2:07 - 2:10and you have to remember
that in the case of Rosetta, -
2:10 - 2:12the spacecraft is in that center pixel.
-
2:12 - 2:16We are only 20, 30, 40 kilometers
away from the comet. -
2:16 - 2:18So what's important to remember?
-
2:18 - 2:23Comets contain the original material
from which our solar system was formed, -
2:23 - 2:26so they're ideal to study the components
-
2:26 - 2:30that were present at the time
when Earth, and life, started. -
2:30 - 2:32Comets are also suspected
-
2:32 - 2:36of having brought the elements
which may have bootstrapped life. -
2:36 - 2:40In 1983, ESA set up
its long-term Horizon 2000 program, -
2:40 - 2:44which contained one cornerstone,
which would be a mission to a comet. -
2:44 - 2:49In parallel, a small mission to a comet,
what you see here, Giotto, was launched, -
2:49 - 2:55and in 1986, flew by the comet of Halley
with an armada of other spacecraft. -
2:55 - 2:59From the results of that mission,
it became immediately clear -
2:59 - 3:04that comets were ideal bodies to study
to understand our solar system. -
3:04 - 3:09And thus, the Rosetta mission
was approved in 1993, -
3:09 - 3:12and originally it was supposed
to be launched in 2003, -
3:12 - 3:15but a problem arose
with an Ariane rocket. -
3:15 - 3:18However, our P.R. department,
in its enthusiasm, -
3:18 - 3:20had already made
1,000 Delft Blue plates -
3:20 - 3:23with the name of the wrong comets.
-
3:23 - 3:26So I've never had to buy any china since.
That's the positive part. -
3:26 - 3:28(Laughter)
-
3:28 - 3:30Once the whole problem was solved,
-
3:30 - 3:33we left Earth in 2004
-
3:33 - 3:36to the newly selected comet,
Churyumov-Gerasimenko. -
3:36 - 3:39This comet had to be specially selected
-
3:39 - 3:41because A, you have to
be able to get to it, -
3:41 - 3:44and B, it shouldn't have been
in the solar system too long. -
3:44 - 3:48This particular comet has been
in the solar system since 1959. -
3:48 - 3:52That's the first time
when it was deflected by Jupiter, -
3:52 - 3:54and it got close enough
to the sun to start changing. -
3:54 - 3:56So it's a very fresh comet.
-
3:57 - 4:00Rosetta made a few historic firsts.
-
4:00 - 4:02It's the first satellite to orbit a comet,
-
4:02 - 4:06and to escort it throughout
its whole tour through the solar system -- -
4:06 - 4:09closest approach to the sun,
as we will see in August, -
4:09 - 4:11and then away again to the exterior.
-
4:11 - 4:14It's the first ever landing on a comet.
-
4:14 - 4:18We actually orbit the comet
using something which is not -
4:18 - 4:19normally done with spacecraft.
-
4:19 - 4:23Normally, you look at the sky and you know
where you point and where you are. -
4:23 - 4:25In this case, that's not enough.
-
4:25 - 4:28We navigated by looking
at landmarks on the comet. -
4:28 - 4:31We recognized features --
boulders, craters -- -
4:31 - 4:35and that's how we know where we are
respective to the comet. -
4:35 - 4:39And, of course, it's the first satellite
to go beyond the orbit of Jupiter -
4:39 - 4:40on solar cells.
-
4:40 - 4:43Now, this sounds more heroic
than it actually is, -
4:43 - 4:48because the technology
to use radio isotope thermal generators -
4:48 - 4:51wasn't available in Europe at that time,
so there was no choice. -
4:51 - 4:53But these solar arrays are big.
-
4:53 - 4:56This is one wing, and these are not
specially selected small people. -
4:56 - 4:58They're just like you and me.
-
4:58 - 5:00(Laughter)
-
5:00 - 5:04We have two of these wings,
65 square meters. -
5:04 - 5:07Now later on, of course,
when we got to the comet, -
5:07 - 5:11you find out that 65 square meters of sail
-
5:11 - 5:16close to a body which is outgassing
is not always a very handy choice. -
5:16 - 5:19Now, how did we get to the comet?
-
5:19 - 5:22Because we had to go there
for the Rosetta scientific objectives -
5:22 - 5:26very far away -- four times the distance
of the Earth to the sun -- -
5:26 - 5:30and also at a much higher velocity
than we could achieve with fuel, -
5:30 - 5:34because we'd have to take six times as
much fuel as the whole spacecraft weighed. -
5:34 - 5:36So what do you do?
-
5:36 - 5:39You use gravitational flybys, slingshots,
-
5:39 - 5:43where you pass by a planet
at very low altitude, -
5:43 - 5:44a few thousand kilometers,
-
5:44 - 5:49and then you get the velocity
of that planet around the sun for free. -
5:49 - 5:51We did that a few times.
-
5:51 - 5:54We did Earth, we did Mars,
we did twice Earth again, -
5:54 - 5:58and we also flew by two asteroids,
Lutetia and Steins. -
5:58 - 6:03Then in 2011, we got so far from the sun
that if the spacecraft got into trouble, -
6:03 - 6:07we couldn't actually
save the spacecraft anymore, -
6:07 - 6:09so we went into hibernation.
-
6:09 - 6:12Everything was switched off
except for one clock. -
6:12 - 6:16Here you see in white the trajectory,
and the way this works. -
6:16 - 6:18You see that from
the circle where we started, -
6:18 - 6:22the white line, actually you get
more and more and more elliptical, -
6:22 - 6:25and then finally we approached the comet
-
6:25 - 6:29in May 2014, and we had to start
doing the rendezvous maneuvers. -
6:29 - 6:34On the way there, we flew by Earth and we
took a few pictures to test our cameras. -
6:34 - 6:36This is the moon rising over Earth,
-
6:36 - 6:38and this is what we now call a selfie,
-
6:38 - 6:42which at that time, by the way,
that word didn't exist. (Laughter) -
6:42 - 6:45It's at Mars. It was taken
by the CIVA camera. -
6:45 - 6:47That's one of the cameras on the lander,
-
6:47 - 6:49and it just looks under the solar arrays,
-
6:49 - 6:53and you see the planet Mars
and the solar array in the distance. -
6:53 - 6:59Now, when we got out
of hibernation in January 2014, -
6:59 - 7:01we started arriving at a distance
-
7:01 - 7:04of two million kilometers
from the comet in May. -
7:04 - 7:08However, the velocity
the spacecraft had was much too fast. -
7:08 - 7:14We were going 2,800 kilometers an hour
faster than the comet, so we had to brake. -
7:14 - 7:16We had to do eight maneuvers,
-
7:16 - 7:18and you see here,
some of them were really big. -
7:18 - 7:24We had to brake the first one
by a few hundred kilometers per hour, -
7:24 - 7:29and actually, the duration of that
was seven hours, -
7:29 - 7:32and it used 218 kilos of fuel,
-
7:32 - 7:36and those were seven nerve-wracking
hours, because in 2007, -
7:36 - 7:39there was a leak in the system
of the propulsion of Rosetta, -
7:39 - 7:41and we had to close off a branch,
-
7:41 - 7:43so the system was actually
operating at a pressure -
7:43 - 7:47which it was never designed
or qualified for. -
7:48 - 7:53Then we got in the vicinity of the comet,
and these were the first pictures we saw. -
7:53 - 7:55The true comet rotation period
is 12 and a half hours, -
7:55 - 7:57so this is accelerated,
-
7:57 - 8:01but you will understand that
our flight dynamics engineers thought, -
8:01 - 8:04this is not going to be
an easy thing to land on. -
8:04 - 8:09We had hoped for some kind
of spud-like thing -
8:09 - 8:11where you could easily land.
-
8:11 - 8:15But we had one hope: maybe it was smooth.
-
8:15 - 8:18No. That didn't work either. (Laughter)
-
8:18 - 8:21So at that point in time,
it was clearly unavoidable: -
8:21 - 8:25we had to map this body
in all the detail you could get, -
8:25 - 8:30because we had to find an area
which is 500 meters in diameter and flat. -
8:30 - 8:34Why 500 meters? That's the error
we have on landing the probe. -
8:34 - 8:37So we went through this process,
and we mapped the comet. -
8:37 - 8:40We used a technique
called photoclinometry. -
8:40 - 8:42You use shadows thrown by the sun.
-
8:42 - 8:45What you see here is a rock
sitting on the surface of the comet, -
8:45 - 8:48and the sun shines from above.
-
8:48 - 8:50From the shadow, we, with our brain,
-
8:50 - 8:54can immediately determine
roughly what the shape of that rock is. -
8:54 - 8:56You can program that in a computer,
-
8:56 - 9:00you then cover the whole comet,
and you can map the comet. -
9:00 - 9:04For that, we flew special trajectories
starting in August. -
9:04 - 9:07First, a triangle
of 100 kilometers on a side -
9:07 - 9:08at 100 kilometers' distance,
-
9:08 - 9:11and we repeated the whole
thing at 50 kilometers. -
9:11 - 9:15At that time, we had seen the comet
at all kinds of angles, -
9:15 - 9:20and we could use this technique
to map the whole thing. -
9:20 - 9:23Now, this led to a selection
of landing sites. -
9:23 - 9:27This whole process we had to do,
to go from the mapping of the comet -
9:27 - 9:31to actually finding
the final landing site, was 60 days. -
9:31 - 9:32We didn't have more.
-
9:32 - 9:34To give you an idea,
the average Mars mission -
9:34 - 9:38takes hundreds of scientists
for years to meet -
9:38 - 9:40about where shall we go?
-
9:40 - 9:42We had 60 days, and that was it.
-
9:42 - 9:45We finally selected the final landing site
-
9:45 - 9:50and the commands were prepared
for Rosetta to launch Philae. -
9:50 - 9:55The way this works is that Rosetta
has to be at the right point in space, -
9:55 - 9:58and aiming towards the comet,
because the lander is passive. -
9:58 - 10:01The lander is then pushed out
and moves towards the comet. -
10:01 - 10:03Rosetta had to turn around
-
10:03 - 10:08to get its cameras to actually look
at Philae while it was departing -
10:08 - 10:10and to be able to communicate with it.
-
10:10 - 10:15Now, the landing duration
of the whole trajectory was seven hours. -
10:15 - 10:18Now do a simple calculation:
-
10:18 - 10:22if the velocity of Rosetta is off
by one centimeter per second, -
10:22 - 10:26seven hours is 25,000 seconds.
-
10:26 - 10:30That means 252 meters wrong on the comet.
-
10:30 - 10:34So we had to know the velocity of Rosetta
-
10:34 - 10:36much better than
one centimeter per second, -
10:36 - 10:40and its location in space
better than 100 meters -
10:40 - 10:43at 500 million kilometers from Earth.
-
10:43 - 10:46That's no mean feat.
-
10:46 - 10:50Let me quickly take you through
some of the science and the instruments. -
10:50 - 10:54I won't bore you with all the details
of all the instruments, -
10:54 - 10:55but it's got everything.
-
10:55 - 10:58We can sniff gas,
we can measure dust particles, -
10:58 - 11:01the shape of them, the composition,
-
11:01 - 11:03there are magnetometers, everything.
-
11:03 - 11:07This is one of the results from
an instrument which measures gas density -
11:07 - 11:09at the position of Rosetta,
-
11:09 - 11:11so it's gas which has left the comet.
-
11:11 - 11:13The bottom graph
is September of last year. -
11:13 - 11:17There is a long-term variation,
which in itself is not surprising, -
11:17 - 11:18but you see the sharp peaks.
-
11:18 - 11:21This is a comet day.
-
11:21 - 11:25You can see the effect of the sun
on the evaporation of gas -
11:25 - 11:28and the fact that the comet is rotating.
-
11:28 - 11:29So there is one spot, apparently,
-
11:29 - 11:31where there is a lot of stuff coming from,
-
11:31 - 11:35it gets heated in the Sun,
and then cools down on the back side. -
11:35 - 11:38And we can see
the density variations of this. -
11:38 - 11:42These are the gases
and the organic compounds -
11:42 - 11:44that we already have measured.
-
11:44 - 11:46You will see it's an impressive list,
-
11:46 - 11:48and there is much, much,
much more to come, -
11:48 - 11:50because there are more measurements.
-
11:50 - 11:54Actually, there is a conference
going on in Houston at the moment -
11:54 - 11:56where many of these results are presented.
-
11:57 - 11:58Also, we measured dust particles.
-
11:58 - 12:01Now, for you, this will not
look very impressive, -
12:01 - 12:05but the scientists were thrilled
when they saw this. -
12:05 - 12:06Two dust particles:
-
12:06 - 12:09the right one they call Boris,
and they shot it with tantalum -
12:09 - 12:11in order to be able to analyze it.
-
12:11 - 12:13Now, we found sodium and magnesium.
-
12:13 - 12:18What this tells you is this is
the concentration of these two materials -
12:18 - 12:20at the time the solar system was formed,
-
12:20 - 12:24so we learned things about
which materials were there -
12:24 - 12:27when the planet was made.
-
12:27 - 12:30Of course, one of the important
elements is the imaging. -
12:30 - 12:33This is one of the cameras of Rosetta,
the OSIRIS camera, -
12:33 - 12:36and this actually was the cover
of Science magazine -
12:36 - 12:39on January 23 of this year.
-
12:39 - 12:42Nobody had expected
this body to look like this. -
12:42 - 12:46Boulders, rocks -- if anything, it looks
more like the Half Dome in Yosemite -
12:46 - 12:48than anything else.
-
12:48 - 12:51We also saw things like this:
-
12:51 - 12:56dunes, and what look to be,
on the righthand side, wind-blown shadows. -
12:56 - 13:00Now we know these from Mars,
but this comet doesn't have an atmosphere, -
13:00 - 13:02so it's a bit difficult to create
a wind-blown shadow. -
13:02 - 13:04It may be local outgassing,
-
13:04 - 13:07stuff which goes up and comes back.
-
13:07 - 13:10We don't know, so there is
a lot to investigate. -
13:10 - 13:12Here, you see the same image twice.
-
13:12 - 13:14On the left-hand side,
you see in the middle a pit. -
13:14 - 13:17On the right-hand side,
if you carefully look, -
13:17 - 13:20there are three jets coming out
of the bottom of that pit. -
13:20 - 13:22So this is the activity of the comet.
-
13:22 - 13:26Apparently, at the bottom of these pits
is where the active regions are, -
13:26 - 13:29and where the material
evaporates into space. -
13:29 - 13:33There is a very intriguing crack
in the neck of the comet. -
13:33 - 13:35You see it on the right-hand side.
-
13:35 - 13:38It's a kilometer long,
and it's two and a half meters wide. -
13:38 - 13:40Some people suggest that actually,
-
13:40 - 13:43when we get close to the sun,
-
13:43 - 13:44the comet may split in two,
-
13:44 - 13:46and then we'll have to choose,
-
13:46 - 13:48which comet do we go for?
-
13:48 - 13:52The lander -- again, lots of instruments,
-
13:52 - 13:57mostly comparable except for the things
which hammer in the ground and drill, etc. -
13:57 - 14:01But much the same as Rosetta, and that is
because you want to compare -
14:01 - 14:04what you find in space
with what you find on the comet. -
14:04 - 14:07These are called
ground truth measurements. -
14:07 - 14:10These are the landing descent images
-
14:10 - 14:12that were taken by the OSIRIS camera.
-
14:12 - 14:16You see the lander getting further
and further away from Rosetta. -
14:16 - 14:20On the top right, you see an image
taken at 60 meters by the lander, -
14:20 - 14:2360 meters above the surface of the comet.
-
14:23 - 14:26The boulder there is some 10 meters.
-
14:26 - 14:30So this is one of the last images we took
before we landed on the comet. -
14:30 - 14:34Here, you see the whole sequence again,
but from a different perspective, -
14:34 - 14:38and you see three blown-ups
from the bottom-left to the middle -
14:38 - 14:42of the lander traveling
over the surface of the comet. -
14:42 - 14:46Then, at the top, there is a before
and an after image of the landing. -
14:46 - 14:50The only problem with the after image is,
there is no lander. -
14:50 - 14:54But if you carefully look
at the right-hand side of this image, -
14:54 - 14:58we saw the lander still there,
but it had bounced. -
14:58 - 14:59It had departed again.
-
14:59 - 15:02Now, on a bit of a comical note here
-
15:02 - 15:07is that originally Rosetta was designed
to have a lander which would bounce. -
15:07 - 15:10That was discarded because
it was way too expensive. -
15:10 - 15:12Now, we forgot, but the lander knew.
-
15:12 - 15:13(Laughter)
-
15:13 - 15:16During the first bounce,
in the magnetometers, -
15:16 - 15:20you see here the data from them,
from the three axes, x, y and z. -
15:20 - 15:22Halfway through, you see a red line.
-
15:22 - 15:24At that red line, there is a change.
-
15:24 - 15:28What happened, apparently,
is during the first bounce, -
15:28 - 15:32somewhere, we hit the edge of a crater
with one of the legs of the lander, -
15:32 - 15:35and the rotation velocity
of the lander changed. -
15:35 - 15:37So we've been rather lucky
-
15:37 - 15:39that we are where we are.
-
15:39 - 15:43This is one of
the iconic images of Rosetta. -
15:43 - 15:47It's a man-made object,
a leg of the lander, -
15:47 - 15:49standing on a comet.
-
15:49 - 15:54This, for me, is one of the very best
images of space science I have ever seen. -
15:54 - 15:59(Applause)
-
15:59 - 16:03One of the things we still have to do
is to actually find the lander. -
16:03 - 16:07The blue area here
is where we know it must be. -
16:07 - 16:11We haven't been able to find it yet,
but the search is continuing, -
16:11 - 16:14as are our efforts to start getting
the lander to work again. -
16:14 - 16:16We listen every day,
-
16:16 - 16:19and we hope that between now
and somewhere in April, -
16:19 - 16:20the lander will wake up again.
-
16:20 - 16:22The findings of what
we found on the comet: -
16:24 - 16:26This thing would float in water.
-
16:26 - 16:29It's half the density of water.
-
16:29 - 16:32So it looks like
a very big rock, but it's not. -
16:32 - 16:36The activity increase we saw
in June, July, August last year -
16:36 - 16:38was a four-fold activity increase.
-
16:38 - 16:40By the time we will be at the sun,
-
16:40 - 16:44there will be 100 kilos
a second leaving this comet: -
16:44 - 16:46gas, dust, whatever.
-
16:46 - 16:48That's 100 million kilos a day.
-
16:50 - 16:52Then, finally, the landing day.
-
16:52 - 16:57I will never forget -- absolute madness,
250 TV crews in Germany. -
16:57 - 16:59The BBC was interviewing me,
-
16:59 - 17:02and another TV crew
who was following me all day -
17:02 - 17:04were filming me being interviewed,
-
17:04 - 17:07and it went on like that
for the whole day. -
17:07 - 17:09The Discovery Channel crew
-
17:09 - 17:11actually caught me
when leaving the control room, -
17:11 - 17:13and they asked the right question,
-
17:13 - 17:17and man, I got into tears,
and I still feel this. -
17:17 - 17:18For a month and a half,
-
17:18 - 17:21I couldn't think about
landing day without crying, -
17:21 - 17:24and I still have the emotion in me.
-
17:24 - 17:27With this image of the comet,
I would like to leave you. -
17:27 - 17:29Thank you.
-
17:29 - 17:34(Applause)
- Title:
- How to land on a comet
- Speaker:
- Fred Jansen
- Description:
-
As manager of the Rosetta mission, Fred Jansen was responsible for the successful 2014 landing of a probe on the comet known as 67P/Churyumov-Gerasimenko. In this fascinating and funny talk, Jansen reveals some of the intricate calculations that went into landing the Philae probe on a comet 500 million kilometers from Earth — and shares some incredible photographs taken along the way.
- Video Language:
- English
- Team:
- closed TED
- Project:
- TEDTalks
- Duration:
- 17:47
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Peter van de Ven
@ 1:44 "deep, frozen" -> "deep frozen"