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Pulsating star sheds light on exoplanet

A team of researchers has developed a new method to measure the internal properties of stars, enabling more accurate assessments of their orbiting planets. By using asteroseismology, they were able to determine the mass and rotation rate of a pulsating star, confirming the existence of an exoplanet in its orbit.

SourceNew York University·JournalProceedings of the National Academy of Sciences·DateJul 29, 2013

New knowledge about early galaxies

A team of researchers studied an early galaxy using the ESO Very Large Telescope and Hubble Space Telescope, determining its size, mass, element content, and star formation rate. The study found that the galaxy contained a high proportion of heavier elements, similar to those in the centre and outer parts of the galaxy.

SourceUniversity of Copenhagen - Niels Bohr Institute·JournalMonthly Notices of the Royal Astronomical Society·DateJul 3, 2013

Hubble unmasks ghost galaxies

Astronomers discover that small dwarf galaxies in the Milky Way contain only a few stars and share the same birth date, indicating they were shut down by reionization. The relic galaxies provide evidence for a transitional phase in the early universe.

SourceNASA/Goddard Space Flight Center·JournalThe Astrophysical Journal Letters·DateJul 10, 2012

The MIRI has 2 faces

MIRI, the Mid-Infrared Instrument on the James Webb Space Telescope, offers unparalleled capabilities for studying distant galaxies, star formation, and planetary systems. Its spectrometer and camera enable scientists to analyze an object's physical properties and image its shape and structure.

Data mining deep space

Bahram Mobasher has received a two-year grant from NASA to compile imaging observations of galaxy surveys taken by the Hubble Space Telescope since 2002. The project aims to provide multi-wavelength data for measuring physical properties of galaxies and studying their formation and evolution.