Skip to main content

NASA's New Mission: UVEX to Study Ultraviolet Sky, Stars, and Stellar Explosions.


This image shows the heart of the barred spiral galaxy NGC 1097, as seen by NASA’s Hubble Space Telescope.



Embarking on a journey to explore the vast realms of space, NASA is gearing up for a groundbreaking mission with UVEX (UltraViolet EXplorer), a space telescope slated to launch in 2030. This mission, designated as NASA’s next Astrophysics Medium-Class Explorer, will conduct an unprecedented all-sky survey, providing invaluable insights into the evolution of galaxies and stars. UVEX's versatility extends to swiftly targeting sources of ultraviolet light, allowing it to capture post-gravitational wave burst explosions resulting from merging neutron stars.


Equipped with an ultraviolet spectrograph, the telescope will also delve into the study of stellar explosions and massive stars, offering a comprehensive understanding of dynamic events shaping our ever-changing universe. Nicola Fox, associate administrator of the Science Mission Directorate at NASA Headquarters, anticipates that UVEX will play a pivotal role in unraveling the mysteries of nearby and distant galaxies, ushering in a new era of cosmic exploration through its wealth of survey data.


The UVEX (UltraViolet EXplorer) telescope's ultraviolet survey is poised to complement data from other wide-survey missions in this decade, including the Euclid mission led by ESA (European Space Agency) with NASA contributions and NASA’s Nancy Grace Roman Space Telescope, scheduled to launch by May 2027. Collaboratively, these missions will craft a modern, multi-wavelength map of the universe, providing a comprehensive understanding of cosmic phenomena.


Mark Clampin, director of the Astrophysics Division at NASA Headquarters, highlighted the significance of the UVEX mission, emphasizing its contribution to creating a lasting legacy archive of data. This innovative telescope will enhance our comprehension of the universe across multiple wavelengths, addressing a crucial priority in Astrophysics – the study of fleeting changes in the cosmos.


Following a meticulous review of proposals, NASA selected the UVEX Medium-Class Explorer concept for development. This decision was based on evaluations by a panel of scientists and engineers, considering NASA's current astrophysics portfolio and available resources. The UVEX mission, set for a two-year duration, is estimated to cost approximately $300 million, excluding launch expenses.


The principal investigator for the UVEX mission is Fiona Harrison at Caltech in Pasadena, California, with collaboration from institutions such as the University of California at Berkeley, Northrop Grumman, and Space Dynamics Laboratory. As part of the Explorers Program, NASA's oldest continuous program, UVEX aims to provide cost-effective access to space for principal investigator-led space science investigations relevant to astrophysics and heliophysics programs.


Since the launch of Explorer 1 in 1958, the program has successfully launched over 90 missions, including groundbreaking endeavors like Uhuru and the Cosmic Background Explorer missions, both contributing to Nobel prizes for their investigators. Managed by NASA's Goddard Space Flight Center for the Science Mission Directorate, the Explorers Program continues to foster a wide range of research and scientific exploration programs encompassing Earth studies, space weather, the solar system, and the universe.

Comments

Popular posts from this blog

James Webb Space Telescope Opens New Frontiers in the Search for Life Beyond Earth.

  This image illustrates a science-based artist’s impression of K2-18 b, a potentially habitable exoplanet 120 light-years away, orbiting a cool dwarf star in its habitable zone. NASA’s James Webb Space Telescope (JWST) is revolutionizing the search for life beyond our solar system, offering humanity its most detailed look yet at distant, potentially habitable worlds. With its extraordinary infrared capabilities, Webb is not only detecting atmospheres on small rocky exoplanets but also probing their chemical makeup in search of biosignatures—clues that could hint at the presence of life. However, scientists caution that context is everything. Atmospheric data alone is not enough to confirm life; understanding a planet’s surface, interior, and broader environment is essential. Even detecting a potential biosignature, such as a gas possibly produced by biological processes, doesn’t equate to discovery. Multiple, independent lines of evidence would be needed to confirm such a find. “F...

Webb Telescope Reveals Tangled Rings and Dusty Chaos in Dying Star System NGC 1514.

  NASA’s James Webb Space Telescope has captured the most detailed image yet of planetary nebula NGC 1514, revealing clumpy dust rings and clear holes in its vibrant pink core using mid-infrared light. A dying star’s final performance has been brought into sharp focus by NASA’s James Webb Space Telescope, revealing a cosmic display of tangled rings, drifting dust, and mysterious holes in the planetary nebula NGC 1514. This mesmerizing structure lies about 1,500 light-years away in the constellation Taurus and has been evolving for at least 4,000 years. At the heart of the nebula are two tightly bound stars, orbiting each other every nine years, their light diffracted in Webb’s images like a celestial jewel. While the stars appear as one in mid-infrared light, they are central to the nebula’s complex architecture. One of these stars, once several times the mass of our Sun, ejected its outer layers in a slow, dense stellar wind as it aged. The other star’s close approach may have twi...

Astronomers have discovered a 'Death Star' black hole in action.

A team of astronomers has studied 16 supermassive black holes that are firing powerful beams into space, tracking where these beams, or jets, are pointing now and where they were aimed in the past, as reported in our latest press release. Using NASA’s Chandra X-ray Observatory and the U.S. National Science Foundation (NSF) National Radio Astronomical Observatory’s (NRAO) Very Large Baseline Array (VLBA), they found that some of the beams have changed directions by large amounts. These two Chandra images show hot gas in the middle of the galaxy cluster Abell 478 (left) and the galaxy group NGC 5044 (right). The center of each image contains one of the sixteen black holes firing beams outwards. Each black hole is located in the center of a galaxy embedded in the hot gas. In the images below, labels and the radio images appear. Ellipses show a pair of cavities in the hot gas for Abell 478 (left), while ellipses indicate two pairs of cavities for NGC 5044 (right). These cavities were carve...