A Spin Through the Inner Solar System

More than 50 years of planetary exploration have yielded a rich harvest of data, including many volumes of pictures. These images have revealed the faces of nearly all the nearby worlds, which have turned out to be both forboding and inviting, alien and familiar. Everywhere there is beauty.

We have enough images, in fact, that for many planets, moons, and small bodies we can construct full, global maps. This has been true for places like Mars for decades. For others, such as Mercury and the asteroid Vesta, it has become possible only in the past few years, thanks to the ongoing work of robotic scouts throughout the Solar System and the dedicated people on Earth who fly them.

Following is a series of short videos showing the worlds of the inner Solar System spinning to show their various faces. With two exceptions, each video resulted from taking thousands of individual observations from spacecraft, and combining the data into a 3D computer model.

This look at the Sun comes from the Solar Dynamics Observatory in orbit around the Earth. It shows the Sun as it appeared over the course of the past few days, as seen by sensors tuned to three different wavelengths of extreme ultraviolet light. Later in the decade, new missions will actually fly close to the Sun for even more detailed shots.

This globe comes from thousands of obesrvations by the MESSENGER spacecraft in orbit around Mercury. MESSENGER carries cameras that can observe many wavelenths of light as it bounces off the planet, in order to spy different minerals on the surface. This map shows greatly exaggerated colors in order to highlight the diversity of geology.

Venus is entirely shrouded in dense clouds, of course, but in the 1990s the Magellan spacecraft mapped the surface anyway using radar. The video highlights two large “continents,” or highlands, Aphrodite Terra and Ishtar Terra, the Maxwell Montes mountain range, and Maat Mons, a large, currently dormant volcano. Notice the motion of the clouds at the beginning. Venus is the one inner planet that rotates “backwards” to the other planets.

This map of the moon comes from thousands of photos sent by the Lunar Reconnaissance Orbiter. Each was taken when the Sun was nearly directly overhead at the moment the image was taken. When all stitched together, they make a globe of striking crispness and clarity.

Here is Mars, showing both the actual relief of its surface features, and a version where the topographical data has been wildly stretched to draw out the planet’s complex landscapes.

Finally, we have Vesta, a tiny place compared to these other worlds, but a giant among the members of the asteroid belt. This rotation is not a computer model, but a series of images stitched together from photos sent by the Dawn spacecraft.

These spinning globes show how much we’ve explored. On the other hand, they serve as a reminder of how much remains unseen. There is no rotating map of the largest asteroid Ceres, or of Pluto. That situation will change next year. However, there are many other worlds in the outer Solar System where there are still blank spaces on the map. Sadly, there are no missions even on the drawing board to explore most of them.

There is still much to do.

This article originally appeared as a guest post on The Planetary Society site.

 

Mission to a Star

There are things that we see every day, but that we don’t really see at all. There are objects so common that we pay them no attention—even the most spectacular ones. At the bright center of all such things, I’d say, is the Sun. When was the last time you noticed it, or thought about what it is?

Here is our very own living star. A spacecraft orbiting the Earth called the Solar Dynamics Observatory (SDO) captured this image…today.

Sun Storms in Extreme Ultraviolet
Sun Storms in Extreme Ultraviolet – The limb of the Sun as it appeared at a wavelength of 171 angstroms, as seen in February, 2014 by the Solar Dynamics Observatory. NASA / GSFC / AIA, EVE, HMI

Looking at the Sun in this wavelength of light is a good way to catch coronal loops, arcs of plasma often larger than the entire Earth, that surge along the Sun’s powerful magnetic field lines. The temperature here reaches about 1 million degrees Kelvin (1.8 million Fahrenheit).

SDO monitors the Sun continually. We can even see a time-lapse movie of the star’s motion over the course of several days, a good reminder that the Sun is much more than a static sphere.

SDO is just one member of a fleet of spacecraft, past and present, that have observed the Sun. But most of these have done so from around or near the Earth (with important exceptions, such as the Helios mission in the 1970s).

For all our watching, we remain in the dark about many of the Sun’s secrets. In the next few years, though, two ambitious new missions will set out for the very heart of the Solar System, and will encounter our star close up.

Solar Orbiter
Solar Orbiter – ESA’s Solar Orbiter spacecraft, slated for launch in 2017. ESA / Astrium

The European Space Agency’s Solar Orbiter spacecraft, in collaboration with NASA, will orbit the sun closer than any other so far, as close as 42 million km, just over a quarter of the distance to Earth. After launch in 2017, Solar Orbiter will swing by Venus and the Earth for gravitational speed boosts before finally reaching operational orbit three-and-a-half years later.

From there, it will chart the innermost regions of the solar system, with clear views of the Sun’s poles.

According to ESA, the spacecraft will be in a great position to observe the links between the sun’s surface, its corona and heliosphere. From the mission site: “Solar Orbiter will be used to examine how the Sun creates and controls the heliosphere, the vast bubble of charged particles blown by the solar wind into the interstellar medium. The spacecraft will combine in situ and remote sensing observations to gain new information about the solar wind, the heliospheric magnetic field, solar energetic particles, transient interplanetary disturbances and the Sun’s magnetic field.”

The spacecraft carries 21 sensors, many of which operate from behind a carefully-designed heat shield that will protect the ship’s workings from temperatures as high as 520°C. A key ingredient in the shield will be ‘Solar Black,’ a type of calcium phosphate derived from burnt bone charcoal, the same material often used in prehistoric cave paintings.

Solar Probe Plus
Solar Probe Plus – NASA’s Solar Probe Plus, slated for launch in 2018. NASA / JHUAPL

The very next year after Solar Obiter departs, another Sun-bound spacecraft is slated for launch. If it successfully completes the mission design reviews now underway, Solar Probe Plus will be the first to actually fly right into the Sun’s atmosphere, the corona. It will pass within 8.5 solar radii of the Sun itself. The goal is to understand how the corona is heated and how the solar wind is accelerated.

Solar Probe Plus will be undertaking quite an odyssey. It will loop around the inner solar system for the better part of a decade, swinging by Venus not once but seven times before finally making a close approach to the Sun in 2024. Once there, the Sun’s tremendous gravity will accelerate the spacecraft to an astounding 724,000 kph (450,000 mph). At that speed you could travel from Los Angeles to San Diego in less than a second. In that place the temperatures, and the views, will be truly terrific.

If they succeed, both of these missions should open our eyes to the Sun in a whole new way.

This article originally appeared as a guest post on The Planetary Society site.