Star and Planet Speeding at 1.2 Million MPH Through Milky Way

February 14, 2025
2 mins read
This artist’s concept visualizes a super-Neptune world orbiting a low-mass star near the center of our Milky Way galaxy. Scientists recently discovered such a system that may break the current record for fastest exoplanet system, traveling at least 1.2 million miles per hour, or 540 kilometers per second.
This artist’s concept visualizes a super-Neptune world orbiting a low-mass star near the center of our Milky Way galaxy. Scientists recently discovered such a system that may break the current record for fastest exoplanet system, traveling at least 1.2 million miles per hour, or 540 kilometers per second. Photo Credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)

A star and its planet are zooming through our galaxy at a mind-boggling speed of 1.2 million miles per hour– roughly twice as fast as our solar system moves through the Milky Way. This discovery could be the fastest-moving planetary system ever discovered.

The discovery provides us a new understanding of how planets and stars move through space. Sean Terry, a scientist at the University of Maryland and NASA, explains their findings: “We think this is a super-Neptune world orbiting a low-mass star.” In simpler terms, they spotted a planet similar to Neptune, circling a star much smaller than our Sun.

This artist’s concept visualizes stars near the center of our Milky Way galaxy. Each has a colorful trail indicating its speed –– the longer and redder the trail, the faster the star is moving. NASA scientists recently discovered a candidate for a particularly speedy star, visualized near the center of this image, with an orbiting planet. If confirmed, the pair sets a record for fastest known exoplanet system.
This artist’s concept visualizes stars near the center of our Milky Way galaxy. Each has a colorful trail indicating its speed –– the longer and redder the trail, the faster the star is moving. NASA scientists recently discovered a candidate for a particularly speedy star, visualized near the center of this image, with an orbiting planet. If confirmed, the pair sets a record for fastest known exoplanet system. Photo Credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)

Scientists found this speedster using a clever method that works like a giant magnifying glass in space. When the star and planet passed in front of a more distant star, their gravity bent and magnified that star’s light– similar to how a magnifying glass makes things appear bigger. This technique, called microlensing, helps astronomers spot objects they can’t see directly.

The star itself is pretty small– only about one-fifth the size of our Sun. Its planet weighs about 29 times more than Earth. They’re both located deep in the crowded centre of our galaxy, about 24,000 light-years away.


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“Finding out how heavy these objects are wasn’t easy,” says David Bennett, a senior research scientist working on the project. His team compared data from 2011 and 2021 using powerful telescopes in Hawaii and a special satellite from the European Space Agency.

If the system’s true speed is high enough, it could potentially escape our galaxy’s gravity and traverse intergalactic space many millions of years in the future. This raises interesting questions about how it got going so quickly in the first place.

This Hubble Space Telescope image shows a bow shock around a very young star called LL Ori. Named for the crescent-shaped wave made by a ship as it moves through water, a bow shock can be created in space when two streams of gas collide. Scientists think a similar feature may be present around a newfound star that could be traveling at least 1.2 million miles per hour, or 540 kilometers per second. Traveling at such a high velocity in the galactic bulge (the central part of the galaxy) where gas is denser could generate a bow shock.
This Hubble Space Telescope image shows a bow shock around a very young star called LL Ori. Named for the crescent-shaped wave made by a ship as it moves through water, a bow shock can be created in space when two streams of gas collide. Scientists think a similar feature may be present around a newfound star that could be traveling at least 1.2 million miles per hour, or 540 kilometers per second. Traveling at such a high velocity in the galactic bulge (the central part of the galaxy) where gas is denser could generate a bow shock. Photo Credit: NASA and The Hubble Heritage Team (STScI/AURA); Acknowledgment: C. R. O’Dell (Vanderbilt University)

To make sure they’ve found what they think they have, the scientists plan to look again next year. As Bennett explains, “We need to check if it moves exactly how we expect it to move.” This careful double-checking is crucial in science.

The planet, despite its record-breaking speed, is too cold for life as we know it. Its small star doesn’t give off enough heat to keep the planet warm, even though the planet would lie at a distance between Venus and Earth if it were in our solar system.

This discovery, published in The Astronomical Journal on February 10, helps scientists understand the different kinds of planetary systems that exist in our galaxy. NASA’s upcoming Nancy Grace Roman Space Telescope will help find more unusual systems like this one, adding to our knowledge of how planets and stars behave in space.

Govind Tekale

Embarking on a new journey post-retirement, Govind, once a dedicated teacher, has transformed his enduring passion for current affairs and general knowledge into a conduit for expression through writing. His historical love affair with reading, which borders on addiction, has evolved into a medium to articulate his thoughts and disseminate vital information. Govind pens down his insights on a myriad of crucial topics, including the environment, wildlife, energy, sustainability, and health, weaving through every aspect that is quintessential for both our existence and that of our planet. His writings not only mirror his profound understanding and curiosity but also serve as a valuable resource, offering a deep dive into issues that are critical to our collective future and well-being.

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