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Astronomers Spot Dwarf Planet Candidate and Vanishing Planet

· Confirmed

Science Desk

In Short: Astronomers have spotted a new dwarf planet candidate, 2026 ED138, which could become the solar system's sixth officially recognized dwarf planet.

2026 ED138 Vera C. Rubin
Photo: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA Image Processing: M. Jurić (UW), D. de Martin & M. Zamani (NSF NOIRLab) / Wikimedia Commons (CC BY 4.0)

Astronomers have spotted a new dwarf planet candidate, 2026 ED138, which could become the solar system's sixth officially recognized dwarf planet. The object has a trail stretching back more than a decade in telescope images, giving researchers a head start in understanding its orbit.

The discovery of 2026 ED138 adds to the ongoing debate about the existence of Planet Nine, a hypothetical ninth planet in the outer solar system. This hypothetical body's existence has been debated for years, with some astronomers suggesting its gravitational effects could explain the peculiar clustering of orbits for a group of extreme trans-Neptunian objects (ETNOs).

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Meanwhile, astronomers have observed a planet that appears to have vanished. The distant world, known as TOI-2535 b, was initially identified as a 'hot Jupiter' where a year takes only 8.25 days. However, recent observations suggest it may have disappeared.

The vanishing planet, TOI-2535 b, was followed by astronomers for years, allowing them to establish its initial characteristics. Its disappearance has left scientists puzzled and has sparked renewed interest in the search for undiscovered planets.

In a separate development, MIT astronomers have discovered a planet, designated BD+05 4868 Ab, located approximately 140 light-years away. This planet is undergoing a process of disintegration, losing a massive amount of material as it orbits its star in just 30.5 hours, forming a long, comet-like debris tail.

Researchers have also found a possible planet in the habitable zone of HD 156295, a hot A-type star about 2,000 K (2,000 °C, 3,600 °F) hotter than the Sun. This discovery is significant as it expands the search for habitable planets to hotter stars, which are less commonly studied.

Based on this candidate, the study estimates that about 10 percent of A-type stars host planets of 5 to 10 Jupiter masses with orbital periods of 1,900 to 2,600 days, with a 68 percent range of 2 to 31 percent.

Lead author Terry Long Phan, an astronomer at National Tsing Hua University in Taiwan, expressed excitement about the potential discovery of Planet Nine. 'It would be really cool if there was some kind of pattern there,' Phan told Science.

However, not all astronomers are convinced. Gary Bernstein, an astronomer at the University of Pennsylvania, noted, 'But I am not convinced, with current data, that you can’t just go with the simplest explanation.'

The outer solar system is getting crowded with theoretical planets, and the search for undiscovered bodies continues.

These findings add to the ongoing exploration of the solar system's outer reaches and the search for new planets.

The observations of 2026 ED138 were taken as part of Hubble’s Outer Planet Atmospheres Legacy (OPAL) program, which has photographed the outer planets annually for more than a decade.

What this adds

The discovery of 2026 ED138 adds to the ongoing debate about the existence of Planet Nine, a hypothetical ninth planet in the outer solar system.

The vanishing planet, TOI-2535 b, was followed by astronomers for years, allowing them to establish its initial characteristics.

The outer solar system is getting crowded with theoretical planets, and the search for undiscovered bodies continues.

These findings add to the ongoing exploration of the solar system's outer reaches and the search for new planets.

Background

Astronomers may have discovered a new dwarf planet candidate and observed a planet that appears to have vanished.

Planet Nine is a hypothetical ninth planet in the outer region of the Solar System. Its gravitational effects could explain the peculiar clustering of orbits for a group of extreme trans-Neptunian objects (ETNOs)—bodies beyond Neptune that orbit the Sun at distances averaging more than 250 astronomical units (AU).

What's confirmed

What's still developing

Sources