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A FRESH LOOK AT KEPLER-444’S ANCIENT PLANETARY SYSTEM

 From  Sky & Telescope,

By  - ASS NOVA,

Edited by - Amal Udawatta,

image of the three stars in the Kepler-444 system

Artist's impression of a star orbited by five planets.
NASA / JPL-Caltech





Astronomers have just taken a closer look at an unusual system containing three stars and at least five planets. In doing so they may have solved a mystery around its formation. The system, known as Kepler-444, is also around 11 billion years old, showing that such systems can be stable over a significant fraction of the universe’s current age.

ONE SYSTEM, THREE STARS, FIVE PLANETS

Located 117 light-years away toward the constellation Lyra, the system is centered around the K0 star Kepler-444 A. Then there’s a tight-knit binary pair of M-type stars orbiting it some 66 astronomical units away (known as Kepler-444 BC). A quintet of planets also orbits Kepler-444 A. All five worlds have radii between 0.4 and 0.7 Earth radius, and every one has an orbital period under 10 days.

image of the three stars in the Kepler-444 system
Typical observation of the central star Kepler-444 A and the binary pair Kepler-444 BC.
Adapted from Zhang et al. 2023

A team of astronomers led by Zhoujian Zhang (University of California, Santa Cruz) recently set about measuring the properties of the crowded system more precisely in several different ways. They used the High Resolution Spectrograph of the Hobby-Eberly Telescope at the McDonald Observatory in Texas to measure Kepler-444 A’s radial velocity. The star’s speed changes as it is pulled around by the other objects in the system. Zhang’s team also measured the relative radial velocities between the binary pair and the central star using the High Resolution Echelle Spectrometer at the W. M. Keck Observatory in Hawaii.

The gravitational pull of its companions causes Kepler-444 A to follow a wiggling path across the night sky. Measuring this changing position is known as astrometry. Zhang’s team conducted astrometric measurements of Kepler-444 A using Keck’s near-infrared imager (NIRC2).

EXPANDING PLANET-FORMING POTENTIAL

Putting all these pieces of the puzzle together, the team arrived at a deeper understanding of the Kepler-444 system and its history. Previous measurements of the system suggested that the binary swings in to within 5 astronomical units of Kepler-444 A. That would have truncated Kepler-444 A’s protoplanetary disk, severely depleting the amount of planet-forming material available. It wasn’t clear how five rocky planets could have formed there.

plot of observed and modeled on-sky separation between the central star and the binary pair.
Top panel: Observed (orange circles) and modeled (green lines) separations between Kepler-444 A and Kepler-444 BC. The black line shows the best-fitting model. Bottom panel: Observed values minus modeled values.
Adapted from Zhang et al. 2023

Now, based on their new measurements, Zhang’s team conclude that the Kepler-444 BC binary only gets within 23 astronomical units of Kepler-444 A. This wider separation would have led to a larger and more massive protoplanetary disk truncated to 8 astronomical units. The team calculate that there would have been 500 Earth masses’ worth of dust available from which to build planets. That compares to just 4 Earth masses of dust using previous estimates. Suddenly the presence of five planets is less perplexing.

As astronomers gain a greater understanding of exoplanets, it’s becoming clear that there’s more than one way to make a solar system.


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