Hubble Zooms in on Shrapnel from an Exploded Star
Not long before the dawn of recorded human history, our distant ancestors would
have witnessed what appeared to be a bright new star briefly blazing in the
northern sky, rivaling the glow of our moon. In fact, it was the titanic
detonation of a bloated star much more massive than our sun. Now, thousands of
years later, the expanding remnant of that blast can be seen as the Cygnus Loop,
a donut-shaped nebula that is six times the apparent diameter of the full moon.
The Hubble Space Telescope was used to zoom into a small portion of that remnant,
called the Veil Nebula. Hubble resolves tangled rope-like filaments of glowing
gases. Supernovae enrich space with heavier elements used in the
formation of future stars and planets and possibly life.
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NASA and Space Telescope Science Institute (STScI) are pleased to announce a new opportunity to apply for observations with the Hubble Space Telescope. Mid-cycle proposals aim to allow the community to follow up on discoveries made since the Cycle 23 proposal deadline. Participation in this program is open to all categories of organizations, both domestic and foreign, including educational institutions, profit and nonprofit organizations, NASA Centers, and other Government agencies. Proposals are limited to no more than 5 orbits. Full details are given at this link.
HST Frontier Fields
Using Director's Discretionary (DD) observing time, HST is undertaking a revolutionary deep field observing program to peer deeper into the Universe than ever before and provide a first glimpse of JWST's universe. These Frontier Fields will combine the power of HST with the natural gravitational telescopes of high-magnification clusters of galaxies. Using both the Wide Field Camera 3 and Advanced Camera for Surveys in parallel, HST will produce the deepest observations of clusters and their lensed galaxies ever obtained, and the second-deepest observations of blank fields (located near the clusters). These images will reveal distant galaxy populations ~10 - 100 times fainter than any previously observed, improve our statistical understanding of galaxies during the epoch of reionization, and provide unprecedented measurements of the dark matter within massive clusters.
Data releases of the already observed clusters are available at the MAST Frontier Fields website.
The Frontier Fields public lensing models have been released and are available on the MAST Frontier Fields Lensing Model website. This website includes interactive tools for examining the lensing maps and obtaining magnifications and uncertainties from a variety of models, given a position and redshift.
For more information about the survey, please see the Frontier Fields website.
Exposure Time Calculators
The ETCs are web-based applications that assist Hubble users in preparing Phase I and Phase II observing proposals. The ETCs calculate exposure times or SNRs for simulated astronomical observations using any of HST's primary instruments:
ACS | COS | STIS | WFC3
Hubble Legacy Archive
The Hubble Legacy Archive (HLA) is designed to optimize science from HST by providing online, enhanced Hubble products and advanced browsing capabilities.