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Salt Clouds on GJ 504b: JWST Reveals a Surprising Atmosphere on the Pink Planet

BY:SpaceEyeNews.

Salt Clouds on GJ 504b Reveal a New Atmospheric Mystery

The James Webb Space Telescope has uncovered an unexpected discovery on one of the most famous planetary companions ever found. Known as the Pink Planet, GJ 504b has fascinated astronomers since its discovery in 2013. Now, new observations have revealed something never seen before in such detail: salt clouds deep within its atmosphere.

The finding is more than a curious weather report. It offers new insight into how cold giant planets and brown dwarfs evolve over billions of years. It also highlights the extraordinary power of the James Webb Space Telescope, which succeeded where some of the world’s largest ground-based observatories struggled.

Most importantly, the discovery of Salt Clouds on GJ 504b may help scientists better understand the atmospheres of distant worlds. At the same time, it raises new questions about the true identity of this unusual object.

Why GJ 504b Stands Out Among Alien Worlds

A World Between Planet and Star

GJ 504b orbits a Sun-like star located about 57 light-years from Earth. Researchers estimate that the object has a mass around 25 times greater than Jupiter.

That mass places it near the boundary between giant planets and brown dwarfs. Brown dwarfs form like stars but never gather enough material to ignite sustained hydrogen fusion in their cores.

Because of this uncertainty, astronomers often classify GJ 504b as a planetary-mass companion rather than a traditional planet.

The Origin of the Pink Planet Name

GJ 504b earned its nickname because of its striking appearance in infrared observations. Processed images showed a vivid pink or magenta color that made it one of the most recognizable directly imaged planetary companions ever discovered.

The unusual appearance quickly turned GJ 504b into a favorite target for follow-up studies.

A Surprisingly Cool Giant

Although it remains far hotter than Earth, GJ 504b is relatively cool compared with many giant exoplanets.

Scientists estimate its temperature at roughly 550 degrees Fahrenheit, or about 290 degrees Celsius.

That temperature makes it one of the coldest planetary-mass companions ever studied in detail through direct imaging. Its cool atmosphere provides an excellent laboratory for understanding how giant worlds change over time.

How JWST Finally Revealed the Secrets of GJ 504b

A Difficult Target for Ground-Based Telescopes

Astronomers have spent years trying to study GJ 504b in greater detail.

The challenge comes from its faintness. The object emits only a small amount of light compared with its much brighter host star.

Previous observations required long observing sessions on powerful telescopes. Even then, researchers struggled to obtain a clear atmospheric spectrum.

JWST Changes the Game

The James Webb Space Telescope approached the challenge differently.

Using its advanced infrared instruments, JWST isolated the faint light coming from GJ 504b while filtering out much of the glare from the parent star.

The result was a detailed spectrum collected in only a few hours.

That spectrum provided a much clearer view of the atmosphere than scientists had ever obtained before.

A Rich Atmospheric Chemistry

The observations revealed several important molecules.

Researchers identified:

  • Water vapor
  • Carbon dioxide
  • Methane
  • Ammonia

These compounds commonly appear in cold giant atmospheres. However, something about the spectrum did not match existing atmospheric models.

Scientists quickly realized that a key ingredient was missing.

Salt Clouds on GJ 504b Solve the Puzzle

When the Models Failed

Atmospheric models allow researchers to compare observations with theoretical predictions.

Initially, the observed spectrum did not fit the expected results.

Some molecular signatures appeared weaker than expected. Others suggested that something was blocking the view into deeper atmospheric layers.

The mismatch indicated that an unknown process was influencing the atmosphere.

Testing Different Cloud Scenarios

Researchers explored several possibilities.

They created simulations using different cloud compositions and atmospheric structures.

Each model attempted to reproduce the observed spectrum.

Many scenarios improved the fit. Yet one explanation stood out from the rest.

Salt Clouds Provide the Missing Piece

The best match came from models that included salt clouds.

These clouds appear deep within the atmosphere and influence how light travels through different layers.

As light passes through the atmosphere, salt clouds partially obscure molecular signatures located below them.

Once researchers included these clouds, the observations became physically consistent.

The discovery of Salt Clouds on GJ 504b marks the first time such clouds have played a critical role in explaining the spectrum of a planetary-mass companion.

Why Salt Clouds Matter

The importance extends beyond a single object.

Atmospheric studies often rely on accurate cloud modeling. Even small errors can produce misleading results.

The discovery suggests that exotic cloud chemistry may be more common than scientists previously thought.

Future studies of cold exoplanets and brown dwarfs may need to consider similar cloud structures.

As a result, Salt Clouds on GJ 504b could become a benchmark case for atmospheric science.

What the Discovery Reveals About the Age of GJ 504b

Cooling Over Billions of Years

Gas giants and brown dwarfs begin their lives extremely hot.

Over time, they slowly lose heat and cool down.

The temperature measured by JWST helped researchers estimate the age of GJ 504b.

Current estimates place its age between 2.5 billion and 4 billion years.

That long cooling history helps explain why the object appears much cooler than many younger giant worlds.

A Window Into Planetary Evolution

Studying older planetary companions provides valuable information.

Researchers can compare young, hot objects with older, cooler ones to understand how atmospheres evolve.

The new observations give scientists a rare opportunity to examine a mature giant world in unprecedented detail.

The Bigger Mystery: What Is GJ 504b?

Evidence Points in Multiple Directions

Even after the discovery of Salt Clouds on GJ 504b, astronomers still face a major question.

Is GJ 504b a giant planet or a brown dwarf?

The answer remains unclear.

Its mass places it near the transition zone between both categories.

Its atmospheric properties also provide mixed clues.

An Atmosphere Rich in Heavy Elements

Researchers found indications that GJ 504b may contain a large amount of elements heavier than hydrogen and helium.

Astronomers often refer to these elements as metals.

High metal content sometimes supports a planetary formation scenario. Giant planets often gather heavy elements while forming inside protoplanetary disks.

However, the evidence is not yet strong enough to settle the debate.

A Mystery for Future Observations

Additional JWST observations may help resolve the question.

Scientists will continue refining atmospheric models and searching for new clues.

Future measurements could reveal more details about the object’s composition, structure, and origin.

For now, GJ 504b remains one of the most intriguing worlds beyond our solar system.

Salt Clouds on GJ 504b Open a New Era of Atmospheric Science

The discovery of Salt Clouds on GJ 504b represents a significant step forward in exoplanet research.

JWST successfully captured a detailed spectrum of a faint and challenging target. The data revealed water vapor, methane, carbon dioxide, ammonia, and an unexpected layer of salt clouds deep within the atmosphere.

Those clouds solved a long-standing modeling problem and provided a new framework for studying cold planetary atmospheres.

Yet the biggest mystery remains unsolved. Scientists still do not know whether GJ 504b formed as a giant planet or as a brown dwarf.

The Pink Planet continues to surprise researchers more than a decade after its discovery. Thanks to JWST, astronomers now understand its atmosphere better than ever before. The next observations may finally reveal what GJ 504b truly is.

Main Sources:

  1. Space.com
    https://www.space.com/astronomy/exoplanets/james-webb-space-telescope-finds-a-salty-surprise-on-famous-pink-planet
  2. Northwestern University News
    https://news.northwestern.edu/stories/2026/06/famous-pink-planet-harbors-a-salty-surprise
  3. Research Paper (arXiv)
    https://arxiv.org/abs/2606.19228
  4. NASA James Webb Space Telescope
    https://science.nasa.gov/mission/webb/