Showing posts with label NGC 1385. Show all posts
Showing posts with label NGC 1385. Show all posts

Saturday, November 18, 2023

Same galaxy, different filters

A spiral galaxy. It has several arms that are mixed together and an overall oval shape. The centre of the galaxy glows brightly. There are bright pink patches and filaments of dark red dust spread across the centre. Credit: ESA/Hubble & NASA, R. Chandar, J. Lee and the PHANGS-HST team

This luminous tangle of stars and dust is the barred spiral galaxy NGC 1385, that lies about 30 million light-years from Earth. The same galaxy was the subject of another Hubble Picture of the Week, but the two images are notably different. This more recent image has far more pinkish-red and umber shades, whereas the former image was dominated by cool blues. This chromatic variation is not just a creative choice, but also a technical one, made in order to represent the different number and type of filters used to collect the data that were used to make the respective images.

It is understandable to be a bit confused as to how the same galaxy, imaged twice by the same telescope, could be represented so differently in two different images. The reason is that — like all powerful telescopes used by professional astronomers for scientific research — Hubble is equipped with a range of filters. These highly specialised components have little similarity to filters used on social media: those software-powered filters are added after the image has been taken, and cause information to be lost from the image as certain colours are exaggerated or reduced for aesthetic effect. In contrast, telescope filters are pieces of physical hardware that only allow very specific wavelengths of light to enter the telescope as the data are being collected. This does cause light to be lost, but means that astronomers can probe extremely specific parts of the electromagnetic spectrum. This is very useful for a number of reasons; for example, physical processes within certain elements emit light at very specific wavelengths, and filters can be optimised to these wavelengths.

Take a look at this week's image and the earlier image of NGC 1385. What are the differences? Can you see the extra detail (due to extra filters being used) in this week’s image?



Friday, April 22, 2022

Black Holes Raze Thousands of Stars to Fuel Growth

NGC 1385 - NGC 1566 - NGC 3344 - NGC 6503
Credit: X-ray: NASA/CXC/Washington State Univ./V. Baldassare et al.; Optical: NASA/ESA/STScI


JPEG (849.3 kb) - Large JPEG (42.2 MB)- Tiff (107.8 MB)- More Images

Tour: Chandra Archive Collection-More Animations



A new survey of over 100 galaxies by NASA's Chandra X-ray Observatory has uncovered signs that black holes are demolishing thousands of stars in a quest to pack on weight. The four galaxies shown in this graphic are among 29 galaxies in the sample that showed evidence for growing black holes near their centers. X-rays from Chandra (blue) have been overlaid on optical images from NASA's Hubble Space Telescope of the galaxies NGC 1385, NGC 1566, NGC 3344, and NGC 6503. The boxes that appear in the roll-over outline the location of the burgeoning black holes.

These new results suggest a somewhat violent path for at least some of these black holes to reach their present size — stellar destruction on a scale that has rarely if ever been seen before.

Astronomers have made detailed studies of two distinct classes of black holes. The smaller variety are "stellar-mass" black holes that typically weigh 5 to 30 times the mass of the Sun. On the other end of the spectrum are the supermassive black holes that live in the middle of most large galaxies, which weigh millions or even billions of solar masses. In recent years, there has also been evidence that an in-between class called "intermediate-mass black holes" (IMBHs) exists. The new study with Chandra could explain how such IMBHs are made through the runaway growth of stellar-mass black holes.

One key to making IMBHs may be their environment. This latest research looked at very dense clusters of stars in the centers of galaxies. With stars in such close proximity, many stars will pass within the gravitational pull of black holes in the centers of the clusters. Theoretical work by the team implies that if the density of stars in a cluster — the number packed into a given volume — is above a threshold value, a stellar-mass black hole at the center of the cluster will undergo rapid growth as it pulls in, shreds and ingests the abundant neighboring stars in close proximity.

Of the clusters in the new Chandra study, the ones with density above this threshold had about twice as many growing black holes as the ones below the density threshold. The density threshold depends also on how quickly the stars in the clusters are moving.

The process suggested by the latest Chandra study can occur at any time in the universe's history, implying that intermediate-mass black holes can form billions of years after the Big Bang, right up to the present day.

A paper describing these results was accepted and appears in The Astrophysical Journal. It is also available online. The authors of the study are Vivienne Baldassare (Washington State University), Nicolas C. Stone (Hebrew University in Jerusalem, Israel), Adi Foord (Stanford University), Elena Gallo (University of Michigan), and Jeremiah Ostriker (Princeton University).

NASA's Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory's Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.








Fast Facts for NGC 1385:

Credit: X-ray: NASA/CXC/Washington State Univ./V. Baldassare et al.; Optical: NASA/ESA/STScI
Scale: Image is about 2.68 arcmin (33,400 light years) across
Category: Black Holes, Normal Galaxies & Starburst Galaxies
Coordinates (J2000): RA 3h 37m 28.33s | -24° 30' 3.22"
Constellation:
Fornax
Observation Dates: Dec 6, 2018
Observation Time: 1 hour 24 minutes
Obs. IDs: 21473
Instrument:
ACIS
Color Code: X-ray: blue; Optical: red, green, and blue
Distance Estimate: About 43 million light years




Fast Facts for NGC 1566:

Credit: X-ray: NASA/CXC/Washington State Univ./V. Baldassare et al.; Optical: NASA/ESA/STScI
Scale: Image is about 2.77 arcmin (25,700 million light years) across
Category: Black Holes, Normal Galaxies & Starburst Galaxies
Coordinates (J2000): RA 4h 20m 0.27s | Dec -54° 56' 12.02"
Constellation:
Dorado
Observation Dates: Dec 3, 2018
Observation Time: 51 minutes
Obs. IDs: 21478
Instrument:
ACIS
Color Code: X-ray: blue; Optical: red, green, and blue
Distance Estimate: About 32 million light years




Fast Facts for NGC 3344:

Credit: X-ray: NASA/CXC/Washington State Univ./V. Baldassare et al.; Optical: NASA/ESA/STScI
Scale: Image is about 2.58 arcmin (46,400 light years) across
Category: Black Holes, Normal Galaxies & Starburst Galaxies
Coordinates (J2000): RA 10h 43m 31.08s | Dec +24° 55" 14.25'
Constellation: Leo Minor
Observation Dates: 2 observations, Jan 25, 2006 & Jan 21, 2013
Observation Time: 13 hours 40 minutes
Obs. IDs: 7087, 15387
Instrument:
ACIS
Color Code: X-ray: blue; Optical: red, green, and blue
Distance Estimate: About 62 million light years




Fast Facts for NGC 6503:

Credit: X-ray: NASA/CXC/Washington State Univ./V. Baldassare et al.; Optical: NASA/ESA/STScI
Scale: Image is about 2.68 arcmin (13,700 light years) across
Category: Black Holes, Normal Galaxies & Starburst Galaxies
Coordinates (J2000): RA 17h 49m 23.4s | Dec +70° 8' 51.12"
Constellation:
Draco
Observation Dates: 2 observations, Mar 23, 2000 & Oct 27, 2000
Observation Time: 4 hours 14 minutes
Obs. IDs: 872, 1640
Instrument:
ACIS
Color Code: X-ray: blue; Optical: red, green, and blue
Distance Estimate: About 18 million light years



Saturday, August 21, 2021

Hubble Views a Galaxy in a ‘Furnace’

NGC 1385
Text credit: European Space Agency (ESA)
Image credit: ESA/Hubble & NASA, J. Lee and the
PHANGS-HST Team
 

This jewel-bright image from the NASA/ESA Hubble Space Telescope shows NGC 1385, a spiral galaxy 68 million light-years from Earth, which lies in the constellation Fornax. The image was taken with Hubble’s Wide Field Camera 3, which is often referred to as Hubble’s workhorse camera thanks to its reliability and versatility. It was installed in 2009 when astronauts last visited Hubble, and 12 years later it remains remarkably productive. 

NGC 1385’s home – the Fornax constellation – is not named after an animal or an ancient god, as are many of the other constellations. Fornax is simply the Latin word for a furnace. The constellation was named Fornax by Nicolas-Louis de Lacaille, a French astronomer born in 1713. Lacaille named 14 of the 88 constellations we still recognize today. He seems to have had a penchant for naming constellations after scientific instruments, including Atlia (the air pump), Norma (the ruler, or set square), and Telescopium (the telescope).


Media Contact:

Claire Andreoli
NASA's Goddard Space Flight Center

 

Source:  NASA/Solar System and Beyond