The type of stars we refer to, which cannot be seen by the naked eye, officially up to now the objects which have suffered the greatest loss of mass. But the spiral structures detected by an international team, including a member who researches at the Instituto de Astrofísica de Canarias (IAC) and at the University of La Laguna (ULL) show that this is not the case. The results of this work are published today in the journal Nature Astronomy.

To celebrate the International Day of Women and Girls in Science, we publish the fourth chapter in the audiovisual series “Girls who broke a glass ceiling looking at the sky”. It will be available in the social networks and the video channels (YouTube and Daylimotion) of the Instituto de Astrofísica de Canarias (IAC), and its objective is to continue drawing attention to the work that women in this Institute carry out, and to encourage the youngest girls to opt for scientific and technical careers.

Because of the International Day of Women and Girls in Science, and International Women’s Day, women scientists and engineers at the Instituto de Astrofísica de Canarias will participate, throughout February and March, in a number of activities to show the role of women in science and to arouse interest in science in young girls.

Two of the planets which are orbiting the star Kepler 107 could be the result of an impact similar to that which affected the Earth to produce the Moon. An international team whose members include a researcher from the Instituto de Astrofísica de Canarias and the University of La Laguna, are publishing the results of this work today in the journal Nature Astronomy.

The result of an agreement signed between the “La Caixa” foundation, the CajaCanaris Foundation and the Instituto de Astrofísica de Canarias (IAC) is that the IAC will train four young people in their workshops and observatories.

It has taken researchers at the Instituto de Astrofísica de Canarias almost three years to produce the deepest image of the Universe ever taken from space, by recovering a large quantity of “lost” light around the largest galaxies in the Hubble Ultra-Deep Field.