This image shows a region of the CANDELS GOODS-South field, which is one of the fields used in this study. This image combines data taken from Hubble Space Telescope's optical and near-infrared cameras, and contains galaxies at a range of distances. The larger galaxies are relatively close by, while the smallest specks hail from the earlier universe. Some of the smallest dots in this image are those used in this study; their light is coming from 0.5 to 1.5 billion years after the Big Bang.
The regular brightness pulsations (red) of white dwarf star PG1149+057 are visibly affected by an outburst (green). Such outbursts have been detected in two pulsating white dwarfs to date, and astronomers plan to hunt for more examples. (Credit: J.J. Hermes/Univ. of Warwick/NASA)
This size and scale of the Kepler-452 system compared alongside the Kepler-186 system and the solar system. Kepler-186 is a miniature solar system that would fit entirely inside the orbit of Mercury.
Scientists using data from NASA's Kepler mission have confirmed the first near-Earth-size planet orbiting in the habitable zone of a sun-like star. The habitable zone is the region around a star where temperatures are just right for water to exist in its liquid form.
The artistic concept compares Earth (left) to the new planet, called Kepler-452b, which is about 60 percent larger. The illustration represents one possible appearance for Kepler-452b — scientists do not know whether the planet has oceans and continents like Earth.
This artist's concept depicts one possible appearance of the planet Kepler-452b, the first near-Earth-size world to be found in the habitable zone of star that is similar to the Sun. The habitable zone is a region around a star where temperatures are right for water — an essential ingredient for life as we know it — to pool on the surface. Scientists do not know if Kepler-452b can support life or not.
Kepler-444 hosts five Earth-sized planets in compact orbits. The planets were detected from the dimming that occurs when they transit the face of their parent star, as shown in this artist's concept. Credit: Tiago Campante/Peter Divine
An animation is also availlable; click to view and download.
The star HD 162826 is probably a "solar sibling," that is, a star born in the same star cluster as the Sun. It was identified by University of Texas at Austin astronomer Ivan Ramirez, in the process of honing a technique to find more solar siblings in the future, and eventually to determine how and where in the Milky Way galaxy the Sun formed.
HD 162826 is not visible to the unaided eye, but can be seen with low-power binoculars. It is 110 light-years away in the constellation Hercules, and appears not far from the bright star Vega in the night sky.
This diagram shows how the diamater of the 17-billion-solar-mass black hole in the heart of galaxy NGC 1277 compares with the orbit of Neptune around the Sun. The black hole is eleven times wider than Neptune's orbit. Shown here in two dimensions, the "edge" of the black hole is actually a sphere. This boundary is called the "event horizon," the point from beyond which, once crossed, neither matter nor light can return.
Credit: D. Benningfield/K. Gebhardt/StarDate
The galaxy NGC 1277 (center) is embedded in the nearby Perseus galaxy cluster. All the ellipticals and round yellow galaxies in the picture are located in this cluster. NGC 1277 is a relatively compact galaxy compared to the galaxies around it. The Perseus cluster is 250 million light years from us.
Credit: David W. Hogg, Michael Blanton, and the SDSS Collaboration
The red circles from left to right represent the measured average color of galaxies at a redshift of 4, 5, 6 and 7, where the bottom axis shows the time since the Big Bang. The light blue bar running through the center of the diagram shows the color of the local galaxy NGC 1705, which contains no dust. When CANDELS astronomers saw that the redshift 7 galaxies in their sample have a similar color as NGC 1705, they derived that those are also dust free. The gradual reddening they observed at lower and lower redshifts reveals that the galaxies are getting dustier with time.