Moving Across the Veil Nebula

This 3-D visualization flies across a small part of the Veil Nebula. It was created using data from the Hubble Space Telescope. It covers part of a the expanding remnant from a star that exploded thousands of years ago, highlighting the emissions from different chemical elements in different layers of gas within the nebula. Emissions from hydrogen, sulfur, and oxygen are shown in red, green, and blue, respectively.

Video Credit: NASA / ESA / and Viz 3D Team, STScI (F. Summers, G. Bacon, Z. Levay, and L. Frattare)

Weighing Sirius B

Sirius A&BAccurately determining the masses of white dwarfs is important to understanding stellar evolution. The Sun will eventually become a white dwarf. White dwarfs are also the source of Type Ia supernova explosions. The method used to calculate a white dwarf’s mass relies on a prediction from Einstein’s theory of General Relativity—that light loses energy when it attempts to escape the gravity of a compact star. This effect is known as the gravitational redshift.

The Hubble image above shows Sirius, the brightest star in our nighttime sky. The bright blob in the center is Sirius A. The dim spot at around 7 o’clock is A’s white dwarf companion star Sirius B. The image of Sirius A was overexposed so that dim Sirius B  could be seen. The X-shaped diffraction spikes and concentric rings around Sirius A and the small ring around Sirius B are artifacts produced within Hubble‘s optical and imaging systems. The two stars revolve around each other every 50 years. Sirius is only 8.6 light-years from Earth, making it the fifth closest star system known.

White dwarfs are the leftover remnants of stars similar to the Sun. They have exhausted their nuclear fuel sources and have collapsed down to a very small size. Sirius B is about 10,000 times dimmer than Sirius A. It’s very faint because of its tiny size, only about 12,000 km in diameter. Sirius B’s weaker light makes it a challenge to study, because its light is swamped in the glare of its brighter companion as seen from telescopes on Earth. Hubble‘s Imaging Spectrograph was able to isolate the light from Sirius B and was able to resolve light from Sirius B being stretched to longer, red-shiftedr wavelengths by the white dwarf’s gravity. Based on those measurements, astronomers have calculated Sirius B’s mass at roughly 98 percent that of the Sun. Further analysis of the star’s spectrum showed that its surface temperature is about 25,000 K.

Image Credit: NASA

Mapping Ceres

CR-7881This color-coded map was assembled using topographic data from the Dawn mission. It shows the highs and lows of the surface of dwarf planet Ceres. It is labeled with names of features that have been approved by the International Astronomical Union. Click on the map to embiggen it.

Image Credit: NASA

An Ultracompact Dwarf Galaxy

M60-UCD1_by_HSTM60-UCD1 is an ultracompact dwarf galaxy. Half of its stellar mass is in the central sphere only 160 light years in diameter. It is probably the densest known galaxy with over one hundred stars per cubic light-year, and it is the smallest and least massive galaxy known to host a central black hole. It is also the most massive ultracompact dwarf galaxy known. It is also one of the oldest galaxies in the universe.

Image Credit: NASA