Personal tools
Log in

Skip to content. | Skip to navigation

INAF

Istituto italiano di astrofisica - national institute for astrophisics

Sections
Ciao
You are here: Home › Dawn's greatest hits

Dawn's greatest hits

A NASA video lists the main scientific activities of the mission, as it leaves the orbit of VESTA and heads towards Ceres.
Dawn's greatest hits

The NASA mission Dawn has left the orbit of Vesta. In a movie compiled for the occasion, NASA tells us the most important scientific results of this year's mission. Scientists, researchers and many team members have gathered virtual social media to celebrate the departure, in an event called "Hasta la Vesta". The next meeting will be with the asteroid Ceres, expected to be in 2015.

Read the full story and watch the video here: http://www.media.inaf.it/2012/09/10/i-greatest-hits-di-dawn/

PLANETARY SYSTEMS, TWO DISTINCT FAMILIES: THE HOST STAR LEAVES ITS SIGNATURE

Oct 13, 2026

PLANETARY SYSTEMS, TWO DISTINCT FAMILIES: THE HOST STAR LEAVES ITS SIGNATURE An international team led by INAF analysed multi-planet systems and found that they split into two distinct families born around different types of stars. The study, published in Nature Astronomy, shows for the first time that the host star's properties determine the architecture and dynamical evolution of the entire planetary system

NGC 362D: TWO RECORD-BREAKING FINDINGS SHED LIGHT ON THE EVOLUTION OF MILLISECOND PULSARS

Sep 30, 2026

NGC 362D: TWO RECORD-BREAKING FINDINGS SHED LIGHT ON THE EVOLUTION OF MILLISECOND PULSARS An INAF- and University of Bologna-led research team has discovered a binary system caught in an exceptionally rare evolutionary stage, consisting of a millisecond pulsar and the youngest white dwarf ever observed in a system of this kind

AN "IMPROBABLE" PLANETARY SYSTEM: COMPACT, COPLANAR, AND SHAPED BY A BROWN DWARF

Jun 17, 2026

AN "IMPROBABLE" PLANETARY SYSTEM: COMPACT, COPLANAR, AND SHAPED BY A BROWN DWARF An international team involving over ten institutions, with a strong participation from ESO and INAF, has characterised TOI-201 c, the transiting brown dwarf with the longest period for which mass has been measured. The study, published today in Nature, reveals a compact, coplanar system in which the presence of a massive, eccentric object redefines the stability boundaries for the inner planets