Thirty years ago, three astronomers and Gene Roddenberry, of Star Trek fame, made the case to Sky & Telescope readers that the orange-hued star 40 Eridani A ought to host Vulcan, Spock's home. Now, a robotic survey has discovered a planet around that very star.
Almost three decades ago, Gene Roddenberry (producer of the Star Trek universe) wrote a letter to Sky & Telescope, along with Harvard-Smithsonian Center for Astrophysics astronomers Sallie Baliunas, Robert Donahue, and George Nassiopoulos. In their Letter to the Editor, they argued that 40 Eridani A — an orange-ish star 16 light-years away — would make the ideal home for Vulcan, the home planet of Science Officer Mr. Spock.
Now, a new discovery puts a little more science into that science fiction assertion.
A Long-ago Letter
In the July 1991 issue, the three astronomers and one movie-maker made the case for what star should be considered Vulcan's home:
The star around which Vulcan orbits was never identified in the original series or in any of the feature films based on it and so has never been officially established. But two candidates have been suggested in related literature.
Two Star Trek books named the star 40 Eridani A as Vulcan's sun, while another publication named Epsilon Eridani instead. However, Roddenberry and the astronomers made an argument for 40 Eridani A:
We prefer the identification of 40 Eridani as Vulcan's Sun because of what we have learned about both stars at Mount Wilson. . . . The HK [Project] observations suggest that 40 Eridani is 4 billion years old, about the same age as the Sun. In contrast Epsilon Eridani is barely 1 billion years old.
Based on the history of life on Earth, life on any planet around Epsilon Eridani would not have had time to evolve beyond the level of bacteria. On the other hand, an intelligent civilization could have evolved over the aeons on a planet circling 40 Eridani. So the latter is the more likely Vulcan sun. . . . Presumably Vulcan orbits the primary star, an orange main-sequence dwarf of spectral type K1. . . . Two companion stars — a 9th magnitude white dwarf and an 11th magnitude red dwarf — orbit each other about 400 astronomical units from the primary. They would gleam brilliantly in the Vulcan sky.
It turns out the letter authors' prediction was right — a world really does orbit the primary star of the three-star 40 Eridani system. (Whether it's home to a logic-based alien society, though, is anyone's guess!)
The world is a super-Earth, the most common type of planet in the galaxy (though a type that's missing from our solar system). At twice Earth's radius and eight to nine times its mass, 40 Eridani b sits on the line that divides rocky super-Earths from gaseous ones. The planet orbits its star every 42 days, putting just inside the system's habitable zone — in other words, where it's nice and hot. At 16 light-years away, it's the closest super-Earth known and therefore a good potential target for followup observations.
The discovery comes courtesy of the Dharma Planet Survey, designed to detect and characterize low-mass planets around bright, nearby stars. Started in 2016 and continuing until 2020, this survey uses a robotic 50-inch telescope on Mount Lemmon to look for planet-induced wobbles in 150 bright stars within 160 light-years of Earth. The spectrograph attached to the scope can measure radial velocities down to 1 meter per second, which enables it to find low-mass planets around these nearby stars.
The discovery will appear in the Monthly Notices of the Royal Astronomical Society. Read the preprint here.