Showing posts with label M1. Show all posts
Showing posts with label M1. Show all posts

Saturday, May 14, 2022

Global Citizen Science Project Finds Over 1700 Asteroid Trails in Hubble Images

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Asteroid Trails Mosaic

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Abell 370 Parallel Field with Asteroids

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Broken Asteroid Trail in NGC 4548

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Asteroid in the Crab Nebula (M1)



Combining artificial intelligence with many keen human eyes, astronomers have found 1701 new asteroid trails in archival data from the NASA/ESA Hubble Space Telescope, consisting of more than 37 000 images that span two decades. The project reflects both Hubble’s value to scientists as an asteroid hunter and how the public can effectively contribute to citizen science initiatives.

On International Asteroid Day in June 2019 an international group of astronomers launched the Hubble Asteroid Hunter, a citizen science project to identify asteroids in archival Hubble data. The initiative was developed by researchers and engineers at the European Science and Technology Centre (ESTEC) and the European Space Astronomy Centre’s Science Data Centre (ESDC), in collaboration with the Zooniverse platform, the world’s largest and most popular citizen science platform, and Google.

The astronomers collectively identified more than 37 000 composite images taken between April 2002 and March 2021 with Hubble’s ACS and WFC3 instruments. With a typical observation time of 30 minutes, asteroid trails appear as curved lines or streaks in these images. Over 11 400 members of the public classified and analysed these images. More than 1000 trails were identified, providing a training set for an automated algorithm based on artificial intelligence. The combination of citizen science and AI resulted in a final dataset containing 1701 trails in 1316 Hubble images. Project participants also tagged various other astronomical objects, such as gravitational lenses, galaxies and nebulae. Volunteers discussed their findings and sought assistance from scientists and other participants via the project’s forum.

Roughly one third of the asteroid trails seen could be identified and attributed to known asteroids in the International Astronomical Union’s Minor Planet Centre, the largest database of Solar System objects. This left 1031 unidentified trails that are faint and likely to be smaller asteroids than those detected in ground-based surveys. The vast majority of these asteroids are expected to be located in the Main Belt between Mars and Jupiter, where asteroids of such small size are as yet poorly studied. These trails could give the astronomers insightful clues about the conditions in the early Solar System when the planets were forming.

The project highlights Hubble’s potential to image faint, previously unknown asteroids and represents a new approach to finding asteroids in astronomical archives spanning decades, which may be effectively applied to other datasets. In addition to illustrating Hubble’s value as an asteroid hunter, it also reinforced the public’s interest in contributing towards scientific endeavours and the value of citizen science efforts.

Next, the project will explore the 1031 streaks of previously unknown asteroids to characterise their orbits and study their properties, such as their sizes and rotation periods. As most of these asteroid streaks were captured by Hubble many years ago, it is not possible to follow them up now to determine their orbits [1]. However, using Hubble, astronomers can use the parallax effect to determine the distance to the unknown asteroids and put constraints on their orbits. As Hubble moves around the Earth, it changes its point of view while observing the asteroid which also moves on its own orbit. By knowing the position of Hubble during the observation and measuring the curvature of the streaks, scientists can determine the distances to the asteroids and estimate the shapes of their orbits. Some of the longer Hubble observations facilitate the measurement of a light curve [2] for the asteroids, from which the team can measure their rotation periods and infer their shapes.



More information

The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

The international team of astronomers in this study consists of S. Kruk (European Space Agency and ​​Max-Planck-Institut für extraterrestrische Physik), P. G. Martín (Universidad Autónoma de Madrid), M. Popescu ( Astronomical Institute of the Romanian Academy), B. Merín (European Space Agency), M. Mahlke (Université Côte d’Azur, Observatoire de la Côte d’Azur), B. Carry (Université Côte d’Azur, Observatoire de la Côte d’Azur), R. Thomson (Google Cloud), S. Karadağ (Google), J. Durán (RHEA for European Space Agency), E. Racero (SERCO for European Space Agency), F. Giordano (SERCO for European Space Agency), D. Baines (Quasar Science Resources for European Space Agency), G. de Marchi (European Space Agency), and R. Laureijs (European Space Agency).

Image credit: ESA/Hubble & NASA, S. Kruk (ESA/ESTEC), Hubble Asteroid Hunter citizen science team, M. Zamani (ESA/Hubble)




Links




Contacts:

Bethany Downer
ESA/Hubble Chief Science Communications Officer
Email:
Bethany.Downer@esahubble.org




Thursday, October 27, 2016

A Dead Star's Ghostly Glow

The eerie glow of a dead star, which exploded long ago as a supernova, reveals itself in this NASA Hubble Space Telescope image of the Crab Nebula. But don't be fooled. The ghoulish-looking object still has a pulse. Buried at its center is the star's tell-tale heart, which beats with rhythmic precision.

Astronomers discovered a real "tell-tale heart" in space, 6,500 light-years from Earth. The "heart" is the crushed core of a long-dead star, called a neutron star, which exploded as a supernova and is now still beating with rhythmic precision. Evidence of its heartbeat are rapid-fire, lighthouse-like pulses of energy from the fast-spinning neutron star. The stellar relic is embedded in the center of the Crab Nebula, the expanding, tattered remains of the doomed star. Credits: NASA and ESA, Acknowledgment: M. Weisskopf/Marshall Space Flight Center

This time-lapse movie of the Crab Nebula, made from NASA Hubble Space Telescope observations, reveals wave-like structures expanding outward from the "heart" of an exploded star. The waves look like ripples in a pond. The heart is the crushed core of the exploded star, or supernova. Called a neutron star, it has about the same mass as the sun but is squeezed into an ultra-dense sphere that is only a few miles across and 100 billion times stronger than steel. This surviving relic is a tremendous dynamo, spinning 30 times a second. The rapidly spinning neutron star is visible in the image as the bright object just below center. The bright object to the left of the neutron star is a foreground or background star. The movie is assembled from 10 Hubble exposures taken between September and November 2005 by the Advanced Camera for Surveys.  Credits: NASA and ESA, Acknowledgment: J. Hester (Arizona State University)


The "heart" is the crushed core of the exploded star. Called a neutron star, it has about the same mass as the sun but is squeezed into an ultra-dense sphere that is only a few miles across and 100 billion times stronger than steel. The tiny powerhouse is the bright star-like object near the center of the image.
This surviving remnant is a tremendous dynamo, spinning 30 times a second. The wildly whirling object produces a deadly magnetic field that generates an electrifying 1 trillion volts. This energetic activity unleashes wisp-like waves that form an expanding ring, most easily seen to the upper right of the pulsar.

The nebula's hot gas glows in radiation across the electromagnetic spectrum, from radio to X-rays. The Hubble exposures were taken in visible light as black-and-white exposures. The Advanced Camera for Surveys made the observations between January and September 2012. The green hue has been added to give the image a Halloween theme.

The Crab Nebula is one of the most historic and intensively studied supernova remnants. Observations of the nebula date back to 1054 A.D., when Chinese astronomers first recorded seeing a "guest star" during the daytime for 23 days. The star appeared six times brighter than Venus. Japanese, Arabic, and Native American stargazers also recorded seeing the mystery star. In 1758, while searching for a comet, French astronomer Charles Messier discovered a hazy nebula near the location of the long-vanished supernova. He later added the nebula to his celestial catalog as "Messier 1," marking it as a "fake comet." Nearly a century later British astronomer William Parsons sketched the nebula. Its resemblance to a crustacean led to M1's other name, the Crab Nebula. In 1928 astronomer Edwin Hubble first proposed associating the Crab Nebula to the Chinese "guest star" of 1054.

The nebula, bright enough to be visible in amateur telescopes, is located 6,500 light-years away in the constellation Taurus.


Ray Villard
Space Telescope Science Institute, Baltimore, Maryland
Villard@stsci.edu
410-338-4514

Editor: Karl Hille