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Measuring the mass of a distant exoplanet requires tracking the changes in light of the host star as the planet’s gravity tugs it slightly — a delicate process. The High Accuracy Radial velocity Planet Searcher for the Northern hemisphere (HARPS-N) is an instrument designed for that purpose. HARPS-N is installed on the Telescopio Nazionale Galileo at the Roque de los Muchachos Observatory on the island of La Palma in the Canary Islands. The instrument provides valuable follow-up observations for the smaller exoplanets identified by NASA’s Kepler/K2 space telescope and other observatories. Astronomers at the Center for Astrophysics | Harvard & Smithsonian are part of the international collaboration operating the instrument. Using the high quality data from HARPS-N, astronomers hope to measure the masses of Earth-like worlds to sufficient accuracy to determine how much these planets resemble ours.

Visit the HARPS-N Website

The Telescopio Nazionale Galileo on La Palma in the Canary Islands at sunset. The High Accuracy Radial velocity Planet Searcher for the Northern hemisphere (HARPS-N) is an instrument on this telescope, designed to find planets orbiting other stars.

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The Telescope and the Science

Astronomers use two complementary methods to discover and characterize exoplanets. The transit method, used by NASA’s Kepler/K2 and TESS spacecraft, provides an estimate of the diameter of the planet. The radial velocity measurements performed by HARPS-N yield the planet’s mass. When both measurements are possible, they reveal the density of the exoplanet, which tells us if the planet is rocky like Earth or gaseous like Neptune.

HARPS-N is a visible-light spectrograph: an instrument designed to measure the spectrum of light from a star to high precision, including the Doppler shift from orbiting exoplanets. As a planet orbits, it tugs the star very slightly. That produces a Doppler shift in the wavelengths of the light emitted by the star, precisely how the sound from a siren on a moving vehicle changes with its speed and direction relative to the listener. For bright stars, HARPS-N can measure the speed of the star’s wobble down to 40 centimeters per second (0.9 miles per hour), which is slower than an average person’s walking speed.

In its first five years of operation from 2012 through 2017, HARPS-N measured the masses of 14 “super-Earth” and “mini-Neptune” exoplanets, which represents about half of the known smaller exoplanets. The goals for the second five years of observation include classifying small rocky exoplanets and identifying an Earth-mass planet in orbit around a Sun-like star.

The HARPS-N spectrograph is a primary instrument on the Telescopio Nazionale Galileo, an Italian-operated 3.58-meter (12-foot) telescope in the Canary Islands off the northwest coast of Africa. This location allows the telescope to view the same part of the sky where Kepler pointed during its primary mission, as well as a significant part of TESS’s observation range. A similar instrument, HARPS, is used on the 3.6-meter European Southern Observatory (ESO) telescope in Chile.

HARPS-N is operated by an international collaboration led by Geneva University, with substantial support from the CfA | Harvard & Smithsonian, the Universities of St. Andrews and Edinburgh in Scotland, the Queens University of Belfast in Northern Ireland, and the Telescopio Nazionale Galileo-INAF Observatory of Italy.