Image Credit: NASA
The Swift satellite has been on orbit for ten years. It was the first project I worked on at Goddard Space Flight Center. I designed and tested the ultra-low-noise power regulator assemblies that run the detector assemblies in the Burst Alert Telescope. I did the circuit design for the variable output high-voltage regulators that provide bias power to the sensors in the BAT detector assemblies. The BAT sensor array is held at a constant temperature (298 K, ± 0.5 K). I designed the pulse-width modulation regulators used in the thermal control system. The same type of PWM is used in the thermal controls for the star trackers which are a part of the satellite’s navigation system. Given that the mission design life was two years, it’s nice to see that my first bits of work are holding up.
Video Credit: NASA
Video Credit: NASA
The MMS mission will expand on the work of the previous THEMIS missions. The four satellites will fly in formation and be able to maintain their alignment with respect to each other by using GPS and sharing their location data with each other. Before I moved on to work on the ASTRO-H mission, I worked on the development of the prototype GPS receivers and other navigation radios for MMS.
Video Credit: NASA
NGC 986 is found in the constellation of Fornax (The Furnace), located in the southern sky. NGC 986 is around 56 million light-years away, and its golden center and barred swirling arms are clearly visible in this image assembled from data captured by Hubble’s Wide Field and Planetary Camera 2. (The stars in the upper right appear a little fuzzy because a gap in the Hubble data was filled in with images from ground-based telescopes. The view is accurate, but the resolution is no match for Hubble.)
Barred spiral galaxies are spiral galaxies with stars forming a central bar-shaped structure. NGC 986 has the characteristic S-shaped structure of this type of galaxy. Young blue stars can be seen dotted through the galaxy’s arms, and the core is also alight with star formation.
Image Credit: NASA / ESA
Ten years ago yesterday, a Delta rocket from Cape Canaveral launched the Swift satellite into orbit. From time to time, I’ve published pictures and videos based on data taken by Swift. Most of it has been related to X-ray astronomy because the instrument that I worked on is an X-ray instrument.
Swift‘s UV Optical Telescope has been used to create the most detailed ultraviolet light surveys ever of the Large and Small Magellanic Clouds, the two closest major galaxies. Nearly a million ultraviolet sources appear in the mosaic of the Large Magellanic Cloud below. It was assembled from 2,200 images taken by the UVOT. The 160-megapixel image (drastically reduced resolution here!) required a cumulative exposure of 5.4 days. The image includes light from 160 to 330 nm. Those UV wavelengths are largely blocked by Earth’s atmosphere. The Large Magellanic Cloud is about 14,000 light-years across.
Image Credits: NASA
An unusual source of light has been found in a galaxy some 90 million light-years away. The object’s odd properties make it a good match for a supermassive black hole ejected from its home galaxy after merging with another giant black hole, or the source, called SDSS1133, might be the remnant of a massive star that erupted for a record period of time before destroying itself in a supernova explosion. Whether it’s a rogue supermassive black hole or the closing act of a rare star, SDSS1133 has been a persistent source for more than 60 years. This sequence of archival astronomical imagery, taken through different instruments and filters, shows that the source is detectable in 1950 and brightest in 2001.
One possible explanation for this source is a very unusual type of star known as a Luminous Blue Variable (LBV). These massive stars undergo episodic eruptions that through off large amounts of matter into space long before they explode. If this be the case, SDSS1133 would have displayed the longest period of LBV eruptions ever observed.
The object could also be a supermassive black hole ejected from its home galaxy after merging with another giant black hole. The collision merger of two galaxies disrupts their shapes and results in new episodes of star formation. If each galaxy possesses a central supermassive black hole, the two black holes will form a bound binary pair at the center of the merged galaxy before ultimately coalescing themselves. The kick may be strong enough to hurl the merged black hole entirely out of its home galaxy, drifting as a rogue through intergalactic space. More likely, it will go into an elongated orbit around the galaxy, retaining the hot gas trapped around it which will continue to shine until all of it is consumed.
This simulation zooms into galaxy Markarian 177 and object SDSS1133 and suggests how they compare with a simulated galaxy collision. When the central black holes in these galaxies combine, a “kick” launches the merged black hole on a wide orbit taking it far from the galaxy’s core.