A few weeks ago I read this in the news:
Here is one of those close-ups.
The BepiColombo spacecraft? I am interested in space missions and have written several blogs about space travel and spacecrafts, but I must have missed this one.
So here is a post about BepiColombo. And about Mercury. And about Gravity Assists.
Let me start with Mercury, the smallest of the eight planets in our solar system. And the fastest, orbiting the Sun in 88 days. Its orbit is the most elliptical of all planets, the distance to the Sun varies between 46 and 70 million km. (For comparison, the similar distances for Earth are 147 and 152 million km).
Mercury is not easy to observe from Earth, because the planet orbits so close to the Sun. For a long time, it was thought that Mercury was tidally locked to the Sun, in the same way as the Moon is tidally locked to Earth. It was only in 1965 that radar observations of Mercury showed that it was actually rotating with a period of 59 days. An Italian scientist, Giuseppe Colombo noticed that this value is 2/3 of the orbital period and suggested that Mercury and the Sun are in a so-called 2:3 resonance, with Mercury rotating 3 times during 2 orbital periods. More about tidal locking and resonances in the appendix.
In the nineteen sixties space travel started, in the USA with the Mariner program from 1962 to 1973. Here are a few of the Mariners. The Mariner 2 was the first spacecraft to reach another planet (Venus), It had not yet a camera on board! The Mariner 4 flew by Mars and took 20(!) pictures of the red planet. .
The Mariner 10 mission had a novelty, after its launch it passed very close to the planet Venus. The gravitation of this planet changed the speed and direction of the Mariner in such a way that it continued its course in the direction of Mercury. This is called a gravity assist, often (confusingly) called a gravitational slingshot. See the appendix for more details.
.In the left diagram you see the effect. Three months after launch the Mariner 10 passes Venus at a distance of less than 6000 km. It brings the spacecraft in an elliptical orbit around the Sun with a period of 176 days. On 29 March it passes Mercury at a distance of 700 km. For the first time in history pictures were taken of Mercury’s surface!, A big surprise was that Mercury had a (weak) magnetic field, so it should have a liquid iron core.
The gravity assist was suggested by the same Giuseppe Colombo and was so successful that it is now a standard procedure for spaceflight.
It took almost 30 years before the next mission to Mercury started. In 2004 the MESSENGER spacecraft was launched and its mission was to go into orbit around Mercury and study its structure and magnetic field. Going into orbit around Mercury is not an easy job because of the strong pull of the Sun. Not less than seven gravity assists were needed to slow down the spacecraft enough, one flyby with Earth itself (!), two with Venus and four with Mercury. Here is a diagram of the flight path. Just to show how complicated it is.
The advantage of gravity assists is that you don’t need fuel to change the course, only minor DSM’s (Deep Space Maneuvers). The “disadvantage” is that it takes considerably more time to reach the target. In this case more than six years.
After this lengthy introduction, let’s go back to the BepiColombo mission. Giuseppe (Bepi) Colombo died in 1984, this mission must have been named BepiColombo in his honor, as he was the first to identify the 2:3 resonance of Mercury and also the first to suggest a gravity assist for the Mariner 10 to reach Mercury..
BepiColombo is a joint mission of the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA). BepiColombo was launched in October 2018. The spacecraft contains two orbiters, one MMO) to study the magnetic fields of Mercury, the other one MPO) will study structure and geology of the planet.
In this animation, you can follow the flight path of BepiColombo (pink) from the launch in 2018 until it goes into orbit around Mercury in 2025. The orbits of Earth, Venus and Mercury are in dark blue, light blue and green, respectively. The spacecraft will use a total of nine(!) gravity assists before it goes into orbit.
As it may be difficult to see where and when the flybys occur, I have taken a few screenshots from a very informative video created by ESA: BepiColombo – orbit and timeline .Worth watching. In the screenshots the flyby is indicted with a circle.
The photo of Mercury at the begining of thos post was, taken during the 2nd flyby of Mercury on 23 June 2022.
When BepiColombo goes into orbit around Mercury, it will have travelled more than 10 billion km. Only then it will deploy the two orbiters.
So we will have to wait more than three years before the two orbiters start collecting scientific data.
Appendix: Tidal locking
As probably everybody knows about tides on earth, we will start there. Twice a day the sea will have a high tide and a low tide. Those tides are caused by the gravitational attraction between Earth and Moon. This force depends on the distance between the two bodies. It is a bit stronger on the side of the earth facing the moon, than on the opposite side, resulting in the tides.
The friction caused by these tidal forces, will slow down the rotation of the Earth, increasing the length of a day. Not much, about 2 milliseconds per century. But when Earth and Moon were formed, about 4.5 billion year ago, the length of a day was much shorter only a few hours.
A similar story holds for the Moon, but here the slowing down has been so effective that for billions of years the moon is “tidally locked”, the rotation if the moon (its “spin) is equal to its orbital period around Earth. The technical term is that the Moon is in a 1:1 spin-orbit resonance with Earth. From Earth we always see the same side of the Moon.
Most other moons in our Solar System are also tidally locked to their planet. For example the four Jupiter moons, discovered by Galileo in 1609.
An interesting case is Pluto (no longer a planet) and its moon Charon. Charon is a large moon and Pluto a small “minor planet”.. Both moon and planet are tidally locked to each other! Here is an animation.
The gravitation of the Sun aldo causes tidal forces on the planets. On Earth we are aware of that, but the Sun’s tidal forces are smaller than those of the moon. During full moon and new moon the two tides enhance each other, the high tide is stronger and called a spring tide. During first and last quarter they work against each other, the high tide is weaker and called a neap tide. See the diagram below
Because Mercury is orbiting so close to the Sun, the tidal forces are a lot stronger. Until 1965 it was thought that Mercury was tidally locked to the Sun, rotating in 88 days, same as the period of its orbit => a 1:1 resonance. Now we know that it is a 2:3 resonance, Mercury rotates faster, 1.5 times during one orbit. The reason is that Mercury’s orbit is quite elliptical, so its (orbital) speed is not constant, moving faster when it is close to the Sun. Here is link to a good explanation: Mercury’s 3:2 Spin-Orbit Resonance. .
The length of a day is commonly defined as the time between successive sunrises or sunsets. 24 hours for Earth, slightly more then the rotation period of 23.9344696 h. With 1:1 tidal locking there is no more sunset/sunrise, the concept of a day has no meaning or you could say that the length of a day is infinite ;-). The animation below shows Mercury orbiting the Sun. The red point represents an observer on Mercury. Note that this observer rotates three times during two orbits. Dawn, midday, dusk and midnight are marked. A day on Mercury takes 176 (earth) days, much longer than the rotation period of 59 (earth) days!
Appendix: Gravity Assists
After launch, a spacecraft will move under the influence of gravitation, primarily the attraction of the Sun. Using the precious fuel on board, it can maneuver a bit to reach its destination. When its course brings it close to a planet, the gravity of this planet can change direction and speed of the spacecraft, without using fuel. Depending on how the spacecraft approaches the planet, its speed can increase or decrease. This use of a planet’s gravity is called a gravity assist or a gravitational slingshot.
Here is a somewhat misleading analogy of a gravity assist. “Space balls” are shot at a train with speed of 30 MPH. If the train is at rest, they bounce back with a speed of 30 MPH. But the train is not at rest, it approaches with a speed of 50 MPH. The balls hit the train now with 30 + 50 = 80 MPH and bounce back with the same speed. For the observer along the rails, the balls now have a speed of 80 + 50 = 130 MPH.
This analogy, from Charley Kohlhase, an important NASA engineer, illustrates a few important points. 1).The balls are interacting with a moving object and 2). the mass of the moving object is so large, that its loss of energy can be neglected.
My own favorite example is that of a tennis player, who hits an incoming ball, before it bounces (a volley). When he keeps his racket still, the ball will bounce back with (about) the same speed (block volley). When he moves his racket forward, the speed will be larger (punch volley), when he moves it backwards, the ball will go back slower (drop volley). In this case his own mass is less than the train, so he will feel the impact of the ball.
In space there are no contact forces, everything moves under the influence of gravity, therefore I always found the analogy unsatisfactory. The influence of gravity on the motion of two bodies in space has been described by Kepler using Newton’s gravitation law. We assume that the mass of one body (a planet) is much larger than the mass of the other one (a spacecraft) Here are a few possible orbits. The red one is part of an ellipse, the green one a parabola and the blue one a hyperbola.
On the Internet you can find numerous videos explaining gravity assist. Pick your choice here. Many of them I found confusing and/or too complicated. So I decided to give it a try myself ;-). Here are three images I have created.
The left image shows the course of a spacecraft under the influence of a planet’s gravitation. It is a hyperbolic orbit, where the speed increases until the spacecraft is closest to the planet (called the periapsis), after which its speed will decrease again. The initial speed and the final one are equal, only the direction has changed (the red arrows). If the planet would be at rest relative to an observer (for example Earth), that would be all.
But that is not the case, the planets move around the Sun. In the second image, a planet moves to the right (blue arrow). The gravitation between spacecraft and planet is still the same (the red arrows) but an outside observer will now see the effect of the two speeds: the green arrows. The change of direction of the red arrows now has a clear effect, the final speed is larger than the initial one: here we have a gravity assist to increase the speed of the spacecraft!. This happens when the spacecraft passes “behind” the planet.
In the last image I have reversed the speed of the planet, so now the spacecraft passes “in front of” the planet. With an opposite effect, now the final speed is less than the initial one, The gravity assist in this case reduces the speed of the spacecraft.
Spacecraft exploring the outer planets have to overcome the gravitation of the sun and will need an “extra push” from gravity assists, passing at the rear of planets. BepiColombo is getting closer to the Sun and has to break to be able to go into orbit around Mercury. Therefore it needs gravity assists, passing in front of a planet, reducing its speed.
For me, this explanation of a gravity assist is satisfactory, I am curious about the opinion of others. Comments are welcome 😉