Maddie Molloy

Maddie Molloy is a news reporter known for her work at the BBC. She has covered a variety of topics including science and technology. Her articles often focus on interesting discoveries and advancements in these fields, as well as their potential impact on society. In addition to her reporting, Maddie is also involved in discussing the challenges faced by individuals with disabilities during the COVID-19 pandemic, particularly related to the use of face coverings.

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The Daily's Verdict

This author is known for its high journalistic standards. The author strives to maintain neutrality and transparency in its reporting, and avoids conflicts of interest. The author has a reputation for accuracy and rarely gets contradicted on major discrepancies in its reporting.

Bias

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Examples:

No current examples available.

Conflicts of Interest

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Examples:

No current examples available.

Contradictions

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Examples:

  • Data from the James Webb Space Telescope revealed the presence of hydrogen sulfide in HD 189733b's atmosphere, a gas that releases a strong sulfuric stench and has never been spotted beyond our solar system before.
  • HD 189733b is a gas giant exoplanet with a size similar to Jupiter but much hotter.
  • The planet has a searing average temperature of 1700 degrees Fahrenheit (926 degrees Celsius) and strong winds that send glass-like silicate particles raining sideways.

Deceptions

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Examples:

No current examples available.

Recent Articles

New Discovery: Hydrogen Sulfide Detected in Exoplanet HD 189733b's Atmosphere

New Discovery: Hydrogen Sulfide Detected in Exoplanet HD 189733b's Atmosphere

Broke On: Monday, 08 July 2024 Scientists using data from the James Webb Space Telescope detected hydrogen sulfide in the atmosphere of exoplanet HD 189733b, located 64 light-years away. This discovery marks the first detection of this gas outside our solar system and sheds light on potential reservoirs of sulfur within planetary atmospheres. The JWST team analyzed infrared light emitted by the gas giant to identify trace amounts of hydrogen sulfide, which has significant implications for understanding exoplanet chemistry and physics.