Roberto Molar

Roberto Molar Candanosa is an artist and a concept designer at Johns Hopkins University. He has contributed to various scientific projects, including the recent study involving the James Webb Space Telescope and exoplanet WASP-107 b. His work involves creating visual representations of scientific concepts, helping to communicate complex ideas to a wider audience.

Biography:  https://phys.org/news/2024-05-webb-telescope-glimpse-exoplanet-interior.html

40%

The overall score is a weighted number that takes into account conflict of interest, bias, deception and other practices that undermines the credibility of the source. It is calculated as:
Analysis.OverallConflictOfInterestScore * 0.3F + Analysis.OverallBiasScore * 0.3F + Analysis.DeceptivenessScore * 0.3F + Analysis.ReadabilityScore * 0.1F

A score that takes into consideration the content for flow, interruptions with ads, and overt search engine optimization techniques that makes the content hard to understand

The Daily's Verdict

This author has a poor reputation for journalistic standards and is not considered a reliable news source.

Bias

0%

Examples:

No current examples available.

Conflicts of Interest

100%

Examples:

No current examples available.

Contradictions

15%

Examples:

  • The exoplanet WASP-107 b has a thousand times less methane than expected and a core 12 times more massive than Earth’s.

Deceptions

0%

Examples:

No current examples available.

Recent Articles

Mystery of Puffy Exoplanet WASP-107b Solved: New Discoveries from JWST and Hubble Reveal Hotter Interior and More Massive Core

Mystery of Puffy Exoplanet WASP-107b Solved: New Discoveries from JWST and Hubble Reveal Hotter Interior and More Massive Core

Broke On: Tuesday, 21 May 2024 Scientists, using data from NASA's JWST and Hubble Space Telescope, reveal new insights into the puffy nature of exoplanet WASP-107b. The discovery of a scarcity of methane in its atmosphere indicates a hotter interior and more massive core. Advanced spectroscopic techniques detect carbon-, oxygen-, nitrogen- and sulfur-bearing molecules for the first time in a transiting exoplanet, shedding light on its composition. The high temperature is attributed to tidal heating from its slightly elliptical orbit around its host star.