Over the past couple weeks, you have surely seen Rosetta and its dusty comet all over the internet, in the news, or on Twitter and other social media sites. It has definitely captured the public imagination. But where did Rosetta come from? How did scientists at the European Space Agency (ESA) manage to accomplish the feat of putting a lander on the surface of a comet hurtling through space? The answer: through a lot of hard work by many people and investment of many resources for many years.
#CometLanding may have been the meme of the week, but it was decades in the making. After Halley’s Comet (1P/Halley) flew by the Earth and was studied by ESA’s Giotto probe, scientists there and at NASA realized that more ambitious missions would be necessary to obtain more detailed information about comets, which contain water and organic materials and could have influenced the origin of life on Earth. ESA’s Science Programme Committee approved the Rosetta mission in November 1993, about 21 years ago. Design and construction took teams of scientists a decade to complete, and then they launched the €1.3 billion flagship spacecraft in 2005 (which was a few months before NASA’s Deep Impact mission sent a probe to collide with a different comet). Following four gravity assists, slingshotting once by Mars and three times by Earth, Rosetta rendezvoused with the comet 67P/Churyumov-Gerasimenko earlier this year. After orbiting for two months, Rosetta was in a position and trajectory to eject Philae, which successfully landed on the comet and made history on 12th November. (See my recent post for more.)
To give another example, for my astrophysics research, I have frequently used data from the Sloan Digital Sky Survey (SDSS), an optical telescope at Apache Point Observatory in New Mexico. The SDSS was first planned in the 1980s, and data collection finally began in 2000. Some have
described the SDSS as one of the most ambitious and influential surveys in the history of astronomy, as it has observed millions of galaxies and quasars, transforming many fields of research, including work on cosmology and the large-scale structure of the universe. It also witnessed the rise of Galaxy Zoo, which with more than 250,000 active “citizen scientists,” has become perhaps the greatest mass participation project ever conceived. Now we prepare for the successors to the SDSS, including ESA’s Euclid mission and the Large Synoptic Survey Telescope, funded by the National Science Foundation (NSF), which are expected to have “first light” in the 2020s.
Scientific research operates on a long time-scale, sometimes longer than the careers of scientists themselves. Scientists make mistakes sometimes, and some projects, large and small, may fail or produce inaccurate results. At times, it may take awhile for scientists to abandon a theory or interpretation insufficiently supported by evidence, and it can be difficult to determine which investigations to pursue that could yield new and fruitful research. Nevertheless, over many years the “self-correcting” nature of the scientific enterprise tends to prevail.
In addition, while the US Congress makes decisions about federal budgets every fiscal year, American scientists depend on predictable stable funding over longer periods in order to successfully complete their research programs. Moreover, school and university students depend on funding and resources for their education. Quality scientific education helps people to become scientifically literate and critical thinkers; as Neil deGrasse Tyson put it, “center line of science literacy…is how you think.” Plus, some students will be inspired by Rosetta and other achievements to pursue careers in science, and we should give them every opportunity to do so.
Events can change rapidly in the 24-hour news cycle, but science and scientists work over years to produce big results like the comet landing. Future missions and ambitious projects for the next few decades are being planned now and need continued support. And to ensure more scientific advancements after that, we need to keep investing in the education of our students—the next generation of scientists.
[Note that this op-ed-like piece is adapted from an assignment I wrote for a science writing class with Lynne Friedmann at UC San Diego.]