Circular Astronomy

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Circular Astronomy

Energy and Structure Formation Cycles in our Universe

  • Protoplanetary Disk Instability Around AB Aurigae (AB Aur)

    Overview AB Aurigae, commonly referred to as AB Aur, is a young star located in the constellation Auriga. It is a Herbig Ae/Be star, which means it is a pre-main-sequence star still in the process of formation. It has a stellar classification of A0Ve, matching an A-type main-sequence star with emission lines in the spectrum.…

    June 24, 2024
  • Pristine Meteorites Give Insights Into the Early Solar System Dynamics

    Researchers investigated the composition of a pristine meteorite and discovered material similar to the outermost protoplanetary disk. This material likely originated in the comet-forming region. New Finding Contrary to previous beliefs, the isotope signature of the comet-forming region appears to be common among outer Solar System bodies. This finding sheds light on the formation and…

    June 23, 2024
  • Formalhaut A with First Asteroid Belt Seen Outside Solar System

    Fomalhaut A is a bright star and was known to the Persian and Arabic Astronomers. The name of the star is Arabic and means “mouth of the fish”. It belongs to a Tripple Star System 25 light-years away from earth. Formalhaut A has several notable characteristics: Fomalhaut Dusty Debris Disk (MIRI Image), James Webb Telescope…

    June 22, 2024
  • HL Tau Protoplanetary Disk Contains More Water Than Earth

    The observations show that there is at least three times more water in the inner disc of the young Sun-like star HL Tauri than in all of Earth’s oceans combined. HL Tau also called HL Tauri is a young T Tauri star located approximately 450 light-years away from earth in the Taurus Molecular Cloud. It…

    June 21, 2024
  • Infant Star SAO 206462 With Protoplanetary Disk 440 Lightyears From Earth

    SAO 206462 (also known as HD 135344B) is a young Herbig F star in the constellation Lupus with a prominent circumstellar protoplanetary disk. The Subaru Telescope captured remarkable images of this system, revealing never-before-seen details of a solar system in the making: 4. Recent high-resolution observations from the James Webb Space Telescope have captured detailed…

    June 20, 2024
  • Young Star HH 211 with Bipolar Jets is a Source of Molecular Emission

    HH 211 is a young bipolar protostellar outflow that provides insights into the early stages of star formation. Here are the key points about HH 211 from the search results: Molecular Emission HH 211 is a prominent source of molecular emission, particularly molecular hydrogen (H2), which traces the outflow’s shocked molecular gas. The molecular emission dominates…

    June 19, 2024
  • Very-Low-Mass Star ISO-Chal 147 with Abundant Hydrocarbons in Protoplanetary Disk

    ISO-Chal-1471 is a young, low-mass star located approximately 600 light-years away from Earth. ISO-Chal 147 is located in the Chamaeleon I star-forming cloud. It is a red dwarf star, which is a type of star that is very common in the Milky Way and burns through fuel slowly. Here are the key points from recent…

    June 18, 2024
  • Dracula’s Chivito (IRAS 23077+6707) Largest Known Protoplanetary Disk with Carbon-Based Molecules

    Dracula’s Chivito, also known as IRAS 23077+6707, is the largest known disk of its kind. It was discovered during a study of active galactic nucleus candidates using images from the Pan-STARRS research project. This edge-on disk completely obscures its central star and is associated with an infrared light source in the same region of the sky.…

    June 17, 2024
  • Star TW Hydrae with Protoplanetary Disc

    TW Hydrae is a young T Tauri star located about 196 light-years away in the constellation Hydra. It is surrounded by a protoplanetary disk. Protoplanetary Disk Chemical Composition The TW Hydrae disk provides a detailed look at the chemical environment where planets are forming, with clear evidence of snow lines, dust evolution, and volatile depletion…

    June 16, 2024
  • Circumstellar Disk Around Star PDS 70

    PDS 70 is a young T Tauri star located about 370 light-years away in the constellation Centaurus. It is surrounded by a protoplanetary disk with a large gap extending from around 65 to 140 AU. Image also shows the PDS 70 cexoplanets. Planetary System Protoplanetary Disk The PDS 70 system provides a rare opportunity to…

    June 14, 2024
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