{"id":626697,"date":"2026-10-10T20:40:11","date_gmt":"2026-10-10T20:40:11","guid":{"rendered":"https:\/\/www.newsbeep.com\/nz\/626697\/"},"modified":"2026-10-10T20:40:11","modified_gmt":"2026-10-10T20:40:11","slug":"a-171-year-old-planetary-mystery-just-took-a-surprising-turn","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/nz\/626697\/","title":{"rendered":"A 171-Year-Old Planetary Mystery Just Took a Surprising Turn"},"content":{"rendered":"

\"Historical<\/a>70 Ophiuchi AB was first identified as a binary star system in the late 1700s by the German astronomer and priest Christian Mayer. This drawing of the system was created by the French astronomer Camille Flammarion in his 1882 book, \u201cLes \u00c9toiles et Les Curiosit\u00e9s du Ciel,\u201d or \u201cStars and Curiosities of the Sky.\u201d Credit: Camille Flammarion<\/p>\n

Coming up empty in a search for giant planets could help astronomers find smaller worlds in the habitable zones of the nearby two-star system 70 Ophiuchi AB.<\/p>\n

Two stars circling each other about 16 light-years from Earth have kept astronomers returning to a possibility first raised in 1855: that a planet might be orbiting nearby. British astronomer William Jacob\u2019s claim that year made the system, 70 Ophiuchi AB, or 70 Oph AB, the host of the first official exoplanet candidate. His claim did not survive scrutiny, but increasingly sophisticated measurements over the following 171 years still could not rule out Jupiter-sized planets in the system\u2019s inner regions.<\/p>\n

University of Michigan researchers have now narrowed that possibility with the most sensitive modern search for giant planets in 70 Oph AB. Their study, published in The Astrophysical Journal, found no large planets and excluded worlds with Jupiter\u2019s mass or greater from specific regions around both stars.<\/p>\n

Stellar activity mimics a planet\u2019s pull<\/p>\n

Astronomers searching for an unseen planet can look for its gravitational pull on a star, which can make the star wobble as the two orbit their shared center of mass. That motion can appear in measurements of radial velocity, the star\u2019s speed toward or away from Earth. Even modern measurements of 70 Oph AB contained a wobble that could have been explained by a Jupiter-sized planet, said Yiting Li, a postdoctoral researcher in U-M\u2019s Department of Astronomy. Changes on a star\u2019s surface can mimic that signal, however, so the measurements left astronomers with competing explanations for what they were seeing.<\/p>\n

\"Binary<\/a>The binary star system 70 Ophiuchi AB, or 70 Oph AB, can be seen near the center of this image taken by the U.S. Naval Observatory in 1937. Astronomers have long been interested in this two-star system and its potential to host planets we have yet to discover. Although researchers led by the University of Michigan didn\u2019t confirm any planets in 70 Oph AB in their latest study, they have set constraints that can aid scientists designing future searches. Credit: Courtesy of the U.S. Naval Observatory Library<\/p>\n

Li assembled a century\u2019s worth of data alongside key new observations from the 6.5-meter (21-foot) Magellan Clay Telescope at Las Campanas Observatory in Chile and the 2.7-meter (8.9-foot) Harlan J. Smith Telescope at McDonald Observatory in Texas. Working with experts from more than a dozen institutions, including NASA\u2019s Jet Propulsion Laboratory and IPAC at the California Institute of Technology, the team reached the sensitivity needed to attribute the wobble to variations on the stars\u2019 surfaces over time. The analysis, supported in part by NASA, removed the need for a planet to explain that signal.<\/p>\n

\u201cYiting assembled an absolutely huge amount of data from all over the world and carefully explored all possibilities,\u201d said Michael Meyer, a senior co-author and chair of U-M\u2019s astronomy department. \u201cIt\u2019s a cautionary tale about how stellar activity can mimic planet signals using the radial velocity.\u201d<\/p>\n

Where Jupiter-mass planets are ruled out<\/p>\n

Around 70 Oph A, the team ruled out planets at least as massive as Jupiter within 5 astronomical units of the star. Around 70 Oph B, that limit extends to half an astronomical unit. An astronomical unit is the distance between Earth and the Sun, so the findings exclude giant planets across a much wider region around the first star. For a system that has been linked to possible planets since the nineteenth century, those boundaries resolve part of a long-standing uncertainty.<\/p>\n

\u201cIt\u2019s a mix of disappointment and excitement,\u201d Li said. \u201cWe\u2019re finding out that there isn\u2019t a Jupiter-sized planet, but we\u2019re also opening the latest chapter on this historic system.\u201d<\/p>\n

\"Historical<\/a>Astronomers first used the visible motion of the stars 70 Ophiuchi A and B to infer that the system might host Jupiter-sized planets close to its stars. New research led by the University of Michigan used more sophisticated techniques\u2014including some of the most sensitive measurements to date\u2014to show that if there are any planets in the system\u2019s interior, they have to be smaller than Saturn. The study also improved the orbit data for the binary system and showed that the two stars had most recently achieved their maximum separation in July 2024. The next time they will reach their minimum separation will be in November 2077. The stars complete an orbit every 88.38 years. Credit: Camille Flammarion<\/p>\n

Saturn-sized planets and smaller worlds could still occupy the system\u2019s habitable zone because the study was not designed to detect them. Within that zone, temperatures could allow liquid water to persist on a rocky planet\u2019s surface, making any such worlds potential targets for future observatories seeking evidence that life exists beyond Earth. Liquid water is a key ingredient for life as we know it, but this search cannot establish whether a rocky planet is there to hold it. \u201cThe study sets an upper limit, not a ban, on planets,\u201d Li said.<\/p>\n

Future missions eye 70 Oph AB<\/p>\n

70 Oph AB offers a nearby place to explore how planets form, evolve, and potentially support life in surroundings different from our single-star solar system. Roughly half of the Milky Way\u2019s stellar systems contain at least two stars, so understanding planets around stellar companions would address a common setting across the galaxy. The University of Michigan describes 70 Oph AB as Earth\u2019s third-closest binary system, behind Alpha Centauri at 4.2 light-years and 61 Cygni at 11.4 light-years.<\/p>\n

The two stars\u2019 orbits are now also among the best characterized in the sky, giving astronomers firmer information to work with as they plan future observations.<\/p>\n

\u201cThe new limit enables us to design optimum search strategies in the future,\u201d Meyer said. \u201cIn fact, the University of Michigan is part of a team studying a space mission called SHERA that will focus on binaries, where this system is one of a handful of targets. 70 Oph AB will certainly be a target of flagship missions, such as NASA\u2019s Habitable World Observatory.\u201d<\/p>\n

The two stars will keep circling each other as astronomers develop the observatories that could search their surroundings for smaller worlds.<\/p>\n

\u201cGiven how prevalent planets are in our universe and in the Milky Way, I would wager that we\u2019ll find there are other planets there,\u201d Li said.<\/p>\n

Reference: \u201cA Century of Radial-velocity and Astrometric Monitoring of 70 Oph AB: New PFS Data and Constraints on Possible Planetary Companions*\u201d by Yiting Li, Michael R. Meyer, Skylar D\u2019Angiolillo, Stephen R. Kane, R. Paul Butler, Stephen A. Shectman, Eric E. Mamajek, Johanna Teske, Jack Lubin, Paul Robertson, Jessie L. Christiansen, Howard Isaacson, Caleb K. Harada, Bradford Holden, William D. Cochran, Michael Endl, Jennifer Burt, Juliette Becker, Alyssa Jankowski, Peter Tuthill, Catherine A. Clark, Rachael M. Roettenbacher, Eric Nielsen, Eduardo Bendek, Armen Tokadjian, William Roberson, Kaitlin M. Kratter, Edwin Bergin, Dave Osip, Jeffrey D. Crane, Alex Davis and Gautam Vasisht, 29 September 2026, The Astrophysical Journal.
DOI: 10.3847\/1538-4357\/ae9f52<\/a><\/p>\n

Additional support for the research was provided by the Heising-Simons Foundation<\/p>\n

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