Rogue Planet Mass and Distance Measured for First Time
Combining Earth- and space-based observations, astronomers measured a rogue planet’s Saturn-like mass and distance, revealing clues about its origin and planetary system ejection.
- In a new study published in Science on Thursday, Subo Dong's team measured a free-floating planet's mass at about 22 percent of Jupiter and its distance at 9,785 light-years.
- Using simultaneous space‑ and ground‑based microlensing observations, the researchers combined Earth and Gaia space telescope views to produce a microlensing parallax that enabled mass and distance calculations.
- The initial microlensing was detected by multiple ground telescopes in Chile, South Africa, and Australia, and Gaia, about 1.5 million kilometers away, also observed it, researchers say.
- Researchers say the measured mass suggests the object was born in a planetary system and was later ejected, and having a measured mass helps estimate masses for other free‑floating planets, Udalski said.
- With NASA's Roman telescope due in 2027, scientists say its ability to survey 1,000 times faster than Hubble could identify hundreds of rogue planets, accelerating future surveys and mission planning.
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28 Articles
Astronomers measure both mass and distance of a rogue planet for the first time
While most planets that we are familiar with stick relatively close to their host star in a predictable orbit, some planets seem to have been knocked out of their orbits, floating through space free of any particular gravitational attachments. Astronomers refer to these lonely planets as "free-floating" or "rogue" planets.
Joint ground- and space-based observations reveal Saturn-mass rogue planet
Simultaneous ground- and space-based observations of a newly discovered free-floating planet have enabled direct measurement of its mass and distance from Earth, according to a new study. The findings offer insights into the diverse and dynamic pathways by which planets can be cast adrift into interstellar space. Although studies to date have only revealed a handful of such free-floating planets, detections are expected to increase in the coming…
A planet, almost as heavy as Saturn, is moving alone through the universe – without a star, without a fixed course. How did it become a loner? And how do you even detect such objects in space?
He still has the bulky name KMT-2024-BLG-0792/OGLE-2024- BLG-0516 and was once thrown out of his orbit around a star. Because a space telescope accidentally spotted him, his mass is now even known.
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