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Young Stellar Objects
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Young Stellar Objects

Young Stellar Objects (YSOs) are stars in their earliest stages of evolution. Just as our Solar System once began as a cloud of dust and gas, these objects form through gravitational collapse. Think of them as "stellar babies" surrounded by a protoplanetary disk. These disks are similar to Saturn's rings but on a much vaster scale. YSOs often eject powerful jets of gas as they struggle to stabilize and ignite thermonuclear fusion. It is a critical phase that determines whether they will become a brilliant star like our Sun or remain hidden within their dusty cocoons.
  • Percentage of Young Stellar Objects within 98.5 light years: 0.02 % (2 from 9522 stars)
  • Average mass of Young Stellar Objects: 10-200% solar mass
  • Average radius of Young Stellar Objects: 50-300% solar radius
  • Average temperature of Young Stellar Objects: 2000-10000 K

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Latest news from Young Stellar Objects

Protoplanet candidate EK Chamaeleontis b identified around a young red dwarf star
icon9. 10. 2026
iconStars | Exoplanets | Young Stellar Obje
Image: Protoplanet candidate EK Chamaeleontis b identified around a young red dwarf star
The search for planets in the very early stages of their formation, known as protoplanets, remains a significant challenge in space observation. A new candidate, designated as EK Cha b, has been observed around the young red dwarf star EK Cha. This object is notable because it provides a rare opportunity to study planetary development within a gas-rich environment. While large gas planets are less common around red dwarf stars compared to larger stars, these cool, small stars represent a common ...
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Inclined planet in the protoplanetary disc of HD 139614 creates shifting shadows
icon6. 10. 2026
iconStars | Exoplanets | Young Stellar Obje
Image: Inclined planet in the protoplanetary disc of HD 139614 creates shifting shadows
An inclined planet orbiting HD 139614 is warping its protoplanetary disc, casting large shadows across the outer regions. New models confirm these shadows and a spiral structure are evidence of the planet's gravitational influence on the surrounding dust....
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Mass measurements of infant planets orbiting the young star V1298 Tau
icon26. 9. 2026
iconStars | Exoplanets | Young Stellar Obje
Image: Mass measurements of infant planets orbiting the young star V1298 Tau
New mass measurements of the infant planets orbiting V1298 Tau reveal that planets b and e are likely gas giants. These findings, based on long-term radial velocity monitoring, suggest higher masses than previously estimated from transit timing observations....
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Variability in the DQ Tau binary system shapes its surrounding planet-forming disk
icon9. 9. 2026
iconStars | Exoplanets | Young Stellar Objects | Planet formatio
Image: Variability in the DQ Tau binary system shapes its surrounding planet-forming disk
The binary system DQ Tau shows that stellar accretion and X-ray activity directly influence its planet-forming disk. Observations reveal that these energy fluctuations shift the disk snowline and change the chemical emission of molecules like water and carbon dioxide....
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Orbital companion dynamics influence the dust disk structure around CQ Tauri
icon1. 8. 2026
iconStars | Exoplanets | Young Stellar Objects | Planet formatio
Image: Orbital companion dynamics influence the dust disk structure around CQ Tauri
CQ Tauri exhibits a complex disk structure with a 25-AU cavity and a dust ring at 53 AU. Simulations suggest that while a Red dwarf companion could explain the inner gap, a massive planet in an outer orbit better matches the observed ring position....
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