海角大神

海角大神 / Text

NASA's decade of sungazing: What have we learned and why does it matter?

Over the course of 10 years, NASA鈥檚 STEREO mission gave us an unprecedented 3D view of our shining star. But astronomers say there鈥檚 still much to learn.

By Joseph Dussault, Staff

After a decade of research, STEREO-A and STEREO-B are finally coming home.

On October 25, 2006, NASA began its Solar Terrestrial Relations Observatory (STEREO) mission. The objective was simple: Obtain stereoscopic images of the sun via two orbiting probes. Having completed their mission, the two crafts are now journeying back to Earth.

It may not sound like much, but it鈥檚 important work 鈥 puns aside, the sun is central to our existence. Without it, our planet would surely be dark and barren: solar activity may have even powered abiogenesis, the process by which life arose from nonliving chemical matter. Over the course of 10 years, NASA鈥檚 STEREO mission gave us an unprecedented 3D view of our shining star. But astronomers say there鈥檚 still much to learn.

The sun takes about 25 days to spin on its axis. In other words, it takes about a month for ground-based researchers to fully observe its surface. That鈥檚 a major problem for astronomers and space weather researchers, because solar storms and sunspots can materialize and dissipate in the span of just a few days.

鈥淵ou can assume how the sun behaves in 3D,鈥 Werner D盲ppen, a heliophysicist at the University of Southern California, tells 海角大神 in an email. 鈥淏ut it is [still] an assumption, since you never see more than half of it. STEREO changed this forever.鈥

In order to capture real-time images of the entire sun, NASA needed two separate vantage points. By positioning one STEREO probe just inside Earth鈥檚 orbit and the other just outside, NASA could observe the sun from three perspectives at once.

In 2007, the mission produced the first ever stereoscopic image of our central star. Four years later, when STEREO-A and STEREO-B were exactly 180 degrees apart, NASA researchers could finally see the whole sun in real time. This unprecedented view gave researchers the data necessary to model certain types of coronal mass ejections.

鈥淭he sun 鈥 directly affects us in ways the planets don鈥檛, so there鈥檚 a much more practical aspect of needing to know more about it,鈥 W. Jeffrey Hughes, a professor of astronomy at Boston University, tells the Monitor in a phone interview. 鈥淭here鈥檚 a whole discipline now called space weather. Magnetic storms can disrupt communications. Magnetic disturbances can affect power grids.鈥

Solar data may also provide some much-needed context to climate studies, experts say.

鈥淥ne of the most pressing scientific questions today is climate change,鈥 Dr. D盲ppen says. 鈥淏y better understanding the sun and its mechanism, we can extrapolate long-term to past and future behavior. Only by assessing the sun's role correctly will we know how much warming is anthropogenic.鈥

In the days of antiquity, the sun was deeply tied to religion. The Incas, Aztecs, and ancient Egyptians 鈥 all critically aware of the sun鈥檚 life-giving power 鈥 considered it a deity. From Malta to Newgrange, prehistoric people built stone megaliths to track its movement and signal the solstices.

According to some ancient biographers, the Greek philosopher Anaxagoras was imprisoned for his 鈥渉eretic鈥 theories about the sun. He proposed that the chariot of Helios, per ancient Greek spiritual belief, was actually a giant flaming mass. Anaxagoras was sentenced to death for this assertion, though he was eventually spared. A few centuries later, Chinese astronomers under the Han Dynasty began keeping meticulous observations of sunspots.

Heliocentrism 鈥 the notion that Earth revolves around the sun, not the other way around 鈥 was first proposed around the same time. But the theory didn鈥檛 pick up traction until the 16th century, when Nicolaus Copernicus explained the theory mathematically. In the coming centuries, luminaries such as Isaac Newton, William Herschel, and Lord Kelvin would reach landmark conclusions about solar radiation and the thermal mechanics of the sun.

In the late 1950s, NASA took a particular interest in our central star. The agency鈥檚 solar satellites, Pioneers 5 through 9, provided the first comprehensive measurements of solar wind and the sun鈥檚 magnetic field. Even then, the sun鈥檚 ability to interrupt communications systems and disrupt electronics wasn鈥檛 fully understood:

In 2018, NASA plans to launch a new solar probe. But this one won鈥檛 just stare into the sun 鈥 it will attempt to 鈥渢ouch鈥 it. Solar Probe Plus will come within 4 million miles of the sun鈥檚 atmosphere, where no spacecraft has gone before, in an effort to better predict coronal activity.

鈥淚t鈥檚 the nature of science that when you find something out, it always raises more questions,鈥 Dr. Hughes says. 鈥淥ne of the big questions in solar physics now is, can we actually say when a solar flare is going to go off?鈥

鈥淚n a society that is reliant on technology, as we are, being able to predict large solar storms is really important,鈥 adds Georgia de Nolfo, deputy project scientist for the STEREO mission, in an email to the Monitor. 鈥淭hat is why missions like STEREO are so important for us. Space weather is the only area of space science to have a national action plan and, quite recently, national security directive from the President.鈥