This
artist's rendition shows one possible appearance for the planet HD
219134b, the nearest rocky exoplanet found to date outside our solar
system. The planet is 1.6 times the size of Earth, and whips around its
star in just three days. Scientists predict that the scorching-hot
planet -- known to be rocky through measurements of its mass and size --
would have a rocky, partially molten surface with geological activity,
including possibly volcanoes. NASA/JPL-Caltech. High Resolution (jpg) - Low Resolution (jpg)
Cambridge, MA - Skygazers at northern latitudes are familiar with the W-shaped star pattern of Cassiopeia the Queen. This circumpolar constellation is visible year-round near the North Star. Tucked next to one leg of the W lies a modest 5th-magnitude star named HD 219134 that has been hiding a secret.
Astronomers have now teased out that secret: a planet in a 3-day orbit that transits, or crosses in front of its star. At a distance of just 21 light-years, it is by far the closest transiting planet to Earth, which makes it ideal for follow-up studies. Moreover, it is the nearest rocky planet confirmed outside our solar system. Its host star is visible to the unaided eye from dark skies, meaning anyone with a good star map can see this record-breaking system.
"Most of the known planets are hundreds of light-years away. This one is practically a next-door neighbor," said astronomer Lars A. Buchhave of the Harvard-Smithsonian Center for Astrophysics (CfA).
"Its proximity makes HD 219134 ideal for future studies. The James Webb Space Telescope and future large ground-based observatories are sure to point at it and examine it in detail," said lead author Ati Motalebi of the Geneva Observatory.
The newfound world, designated HD 219134b, was discovered using the HARPS-North instrument on the 3.6-meter Telescopio Nazionale Galileo in the Canary Islands. The CfA is a major partner with the Geneva Observatory on the HARPS-North Collaboration, which includes several other European partners.
HARPS-North detects planets using the radial velocity method, which allows astronomers to measure a planet's mass. HD 219134b weighs 4.5 times the mass of Earth, making it a super-Earth.
With such a close orbit, researchers realized that there was good possibility the planet would transit its star. In April of this year they targeted the system with NASA's Spitzer Space Telescope. At the appropriate time, the star dimmed slightly as the planet crossed the star's face. Measuring the depth of the transit gave the planet's size, which is 1.6 times Earth. As a result, the team can calculate the planet's density, which works out to about 6 g/cm3. This shows that HD 219134b is a rocky world.
But wait, there's more! The team detected three additional planets in the system using radial velocity data. A planet weighing at least 2.7 times Earth orbits the star once every 6.8 days. A Neptune-like planet with 9 times the mass of Earth circles in a 47-day orbit. And much further out, a hefty fourth world 62 times Earth's mass orbits at a distance of 2.1 astronomical units (200 million miles) with a "year" of 1,190 days. Any of these planets might also transit the star, so the team plans to search for additional transits in the months ahead.
HD 219134 is an orange Type K star somewhat cooler, smaller and less massive than our Sun. Its key measurements have been pinned down very precisely, which thus allows a more precise determination of the properties of its accompanying planets.
This discovery came from the HARPS-North Rocky Planet Search, a dedicated survey examining about 50 nearby stars for signs of small planets. The team targeted nearby stars because those stars are brighter, which makes follow-up studies easier. In particular, additional observations might allow the detection and analysis of planetary atmospheres.
HD 219134 was one of the closest stars in the sample, so it was particularly lucky to find that it hosts a transiting planet. This system now holds the record for the nearest transiting exoplanet. As such, it likely will be a favorite for researchers for years to come.
The paper describing this research has been accepted for publication in the journal Astronomy & Astrophysics.
Headquartered in Cambridge, Mass., the Harvard-Smithsonian Center for Astrophysics (CfA) is a joint collaboration between the Smithsonian Astrophysical Observatory and the Harvard College Observatory. CfA scientists, organized into six research divisions, study the origin, evolution and ultimate fate of the universe.
For more information, contact:
Christine Pulliam
Media Relations Manager
Harvard-Smithsonian Center for Astrophysics
617-495-7463
cpulliam@cfa.harvard.edu
