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Astronomers Map the Universe With the Brightest Objects in the Sky

Astronomers with the international, multi-institutional Sloan Digital Sky Survey have used the world's largest sample of quasars to map a previously uncharted region of the universe. Quasars are brilliant, distant points of light powered by supermassive black holes at their centers. As matter and energy fall into a quasar’s black hole, they heat up to incredible temperatures and glow brighter than anything else in the universe. That luminescence is captured by a 2.5 meter-diameter telescope on a mountaintop in New Mexico here on Earth.

Kyle Dawson, associate professor

Kyle Dawson, associate professor of physics and astronomy at the University of Utah, is the lead U.S. scientist on this cosmology project. He led the team to prepare and acquire the data for more than 147,000 quasars using the telescope at the Apache Point Observatory in Sunspot, New Mexico. His group oversaw the survey planning, observations, and software that turned the photons of light emitted by the quasars into data that can be understood by the rest of the team.

“Quasars are like bright, little lighthouses spread around the galaxy,” says Dawson. “We use them like beacons to see where matter is distributed in the universe.”

From the Sloan Digital Sky Survey (SDSS) website.

"Astronomers with the Sloan Digital Sky Survey (SDSS) have created the first map of the large-scale structure of the Universe based entirely on the positions of quasars. Quasars are the incredibly bright and distant points of light powered by supermassive black holes.

“Because quasars are so bright, we can see them all the way across the Universe,” said Ashley Ross of the Ohio State University, the co-leader of the study. “That makes them the ideal objects to use to make the biggest map yet.”

The amazing brightness of quasars is due to the supermassive black holes found at their centers. As matter and energy fall into a quasar’s black hole, they heat up to incredible temperatures and begin to glow. It is this bright glow that is detected by a dedicated 2.5-meter telescope here on Earth.

A slice through largest-ever three-dimensional map of the Universe. Earth is at the left, and distances to galaxies and quasars are labelled by the lookback time to the objects (lookback time means how long the light from an object has been traveling to reach us here on Earth). The locations of quasars (galaxies with supermassive black holes) are shown by the red dots, and nearer galaxies mapped by SDSS are also shown (yellow).
The right-hand edge of the map is the limit of the observable Universe, from which we see the Cosmic Microwave Background (CMB) – the light “left over” from the Big Bang. The bulk of the empty space in between the quasars and the edge of the observable universe are from the “dark ages”, prior to the formation of most stars, galaxies, or quasars. Click on the image for a larger version.
Image Credit: Anand Raichoor (École polytechnique fédérale de Lausanne, Switzerland) and the SDSS collaboration

“These quasars are so far away that their light left them when the Universe was between three and seven billion years old, long before the Earth even existed,” said Gongbo Zhao from the National Astronomical Observatories of Chinese Academy of Sciences, the study’s other co-leader.

To make their map, scientists used the Sloan Foundation Telescope to observe an unprecedented number of quasars. During the first two years of the SDSS’s Extended Baryon Oscillation Spectroscopic Survey (eBOSS), astronomers measured accurate three-dimensional positions for more than 147,000 quasars.

The telescope’s observations gave the team the quasars’ distances, which they used to create a three-dimensional map of where the quasars are. But to use the map to understand the expansion history of the Universe, they had to go a step further, using a clever technique involving studying “baryon acoustic oscillations” (BAOs). BAOs are the present-day imprint of sound waves which travelled through the early Universe, when it was much hotter and denser than the Universe we see today. But when the Universe was 380,000 years old, conditions changed suddenly and the sound waves became “frozen” in place. These frozen waves are left imprinted in the three-dimensional structure of the Universe we see today.

The good news about these frozen waves – the original baryon acoustic oscillations – is that the process that produced them is simple. Thus, we have a good understanding of what BAOs must have looked like at that ancient time. When we look at the three-dimensional structure of the Universe today, it contains these same BAOs grown out to a huge scale by the expansion of the Universe. The observed size of the BAO can be used as a “standard ruler” to measure distances. Just as by using the apparent angle of a meter stick viewed from the other side of a football field, you can estimate the length of the field. “You have meters for small units of length, kilometres or miles for distances between cities, and we have the BAO scale for distances between galaxies and quasars in cosmology,” explained Pauline Zarrouk, a PhD student at the Irfu/CEA, University Paris-Saclay, who measured the projected BAO scale.

Astronomers from the SDSS have previously used the BAO technique on nearby galaxies and then on intergalactic gas distributions to push this analysis farther and farther back in time. The current results cover a range of times where they have never been observed before, measuring the conditions when the Universe more than two billion years before the Earth formed.

The results of the new study confirm the standard model of cosmology that researchers have built over the last twenty years. In this standard model, the Universe follows the predictions of Einstein’s General Theory of Relativity — but includes components whose effects we can measure, but whose causes we do not understand. Along with the ordinary matter that makes up stars and galaxies, the Universe includes dark matter – invisible yet still affected by gravity – and a mysterious component called “Dark Energy.” Dark Energy is the dominant component at the present time, and it has special properties that cause the expansion of the Universe to speed up.

“Our results are consistent with Einstein’s theory of General Relativity” said Hector Gil-Marin, a researcher from the Laboratoire de Physique Nucléaire et de hautes Énergies in Paris who undertook key parts of the analysis. “We now have BAO measurements covering a range of cosmological distances, and they all point to the same thing: the simple model matches the observations very well.”

Even though we understand how gravity works, we still do not understand everything – there is still the question of what exactly dark energy is. “We would like to understand Dark Energy further,” said Will Percival from the University of Portsmouth, who is the eBOSS survey scientist. “Surveys like eBOSS are helping us to build up our understanding of how dark energy fits into the story of the Universe.”

The eBOSS experiment is still continuing, using the Sloan Telescope at Apache Point Observatory in New Mexico, USA. As astronomers with eBOSS observe more quasars and nearby galaxies, the size of their map will continue to increase. After eBOSS is complete, a new generation of sky surveys will begin, including the Dark Energy Spectroscopic Instrument (DESI) and the European Space Agency Euclid satellite mission. These will increase the fidelity of the maps by a factor of ten compared with eBOSS, revealing the Universe and Dark Energy in unprecedented detail."

Kyle Dawson's post-doctoral researchers whom also worked on this project are:
Julian Bautista: oversees development, maintenance, and operations of the software to process all of the spectra from eBOSS
Vivek Mariappan: coordinates all preparation, operations and observing planning for eBOSS

Read the full press release on the SDSS website"


Patrick Wiggins Discovers Bright Supernova in ‘Fireworks Galaxy’ NGC 6946

New Supernova is Bright Enough to Spot from Earth

Confirmed supernova, "SN 2017aew", can be seen on the top right side of the "Fireworks Galaxy" in the center of this animation. Photo Credit: Patrick Wiggins

On May 13, 2017, "Phun With Physics" Outreacher and NASA solar system ambassador to Utah, Patrick Wiggins spotted something unusual in the sky. He was looking at the spiral galaxy NGC 6946 (the "Fireworks Galaxy") in Cygnus, over 22 million light-years away from his telescope and home near Erda, UT. He noticed a bright spot that he hadn't seen before. By comparing what he what he was seeing with earlier photographs taken of the same galaxy, he realized he was witnessing a star explode.

Named "SN 2017aew", Patrick Wiggins' discovery was confirmed on May 14th by two astronomers: Dr. Subo Dong from the Kavli Institute for Astronomy and Astrophysics (KIAA) at Peking University, and Dr. Krzysztof Z. Stanek from The Ohio State University, both experts in supernovae.

When a star goes supernova, it is one of the largest, and most impressive astronomical events in space. Situated between a nova and a hypernova in terms of total energy, a supernova occurs when a star's core changes in some manner. This can be due to either a white dwarf gaining too much mass from another star orbiting around the same point in a binary star system until the white dwarf's core is so dense that it collapses due to the overwhelming gravitational force (known as a Type I Supernova), or a massive star (many, many times larger than our own sun) reaches the end of its life and runs out of nuclear fuel. The star's core collapses from its own staggering gravitational forces and explodes (a Type II Supernova). In both cases, these supernovae are astoundingly bright for a time - bright enough to be seen by amateur and professional astronomers alike - until they expend their energy and their bright light begins to fade over the next few months.

Patrick Wiggins
Longtime Utah astronomy educator Patrick Wiggins in 2014. Photo Credit: Bill Dunford

This most recent discovery, SN 2017aew, has been confirmed to be a Type II supernova.

This is the third supernova discovery for Patrick Wiggins. He also discovered "SN 2015Q" in the NGC 3888 galaxy in Ursa Major in 2015. In 2014, supernova "SN2014G" was discovered independently by both Koichi Itagaki in Japan, and Patrick Wiggins.

In addition, Patrick Wiggins has discovered a whole host of astronomical events in space, including an asteroid he discovered in 2008, which the International Astronomical Union named "Univofutah", at Patrick's request, to honor the University of Utah. Wiggins' work has earned him many accolades, including the prestigious Distinguished Public Service Medal, NASA's highest civilian honor.

This story is still developing and will be updated as new information becomes available. Stay tuned.


Commencement & Convocation Information 2017

From the Office of the Registrar & the College of Science


University Commencement will be held on Thursday, May 4, 2017 at 6:30pm in the Jon M. Huntsman Center (Map). Candidates for graduation in the summer 2016, fall 2016, spring 2017, or summer 2017 terms may attend.

Commencement is open to the public and free to attend. No tickets or RSVP required. The world-renowned mountain climber, filmmaker, author, philanthropist and Universityof Utah alum Conrad Anker will deliver the commencement address. Honorary Degrees will be awarded to Conrad Anker and Gail Miller.For more information, please visit the Commencement Ceremony page. Those who are unable to attend commencement can watch it streamed live on or online via

For those of you attending or participating in graduation ceremonies this spring, here's some important information.


(For the entire campus where the VIPs speak)
Thursday, May 4, 2017
Jon M. Huntsman Center (Map)

  • 5:00 pm - Graduates assemble in the Parking Terrace west of the Huntsman Center dressed in cap and gown
  • 5:30 pm - Guests should be seated
  • 5:45 pm - Procession begins
  • 6:30 pm - Commencement ceremony begins


(Where your name is called and you walk across the stage)
College of Science (Click here for other colleges' date, time and location)
Thursday, May 4, 2017
Jon M. Huntsman Center (Map)
More info

  • 7:15 - 7:45 am - Graduates assemble outside Jon M. Huntsman Center (see the link above for additional details)
  • 9:00 am - Convocation ceremony begins
  • 11:00 am College of Science Reception at the S.J. Quinney Law Building, 6th Floor, Room 6623 (see below for additional details)


Following the Convocation, graduates and their guests are invited to a reception for the College of Science Class of 2017. Lunch will be served. This reception will be held:
Thursday, May 4, 2017
11:00 a.m. - 1:00 p.m.
Law Building, 6th Floor, Room 6623 (map)


Convocation will also be streamed live online so forward these links to family and friends who want to view it, but can't attend:
On-demand streaming of the College of Science Convocation will be available here.
The live stream link will be available here.


Campus parking lots may be used at no charge during commencement and convocation ceremonies. Please see the commencement parking map for parking locations as well as shuttle and TRAX stops. Additionally, since campus parking is limited, we encourage the use of UTA TRAX on these days. The use of TRAX while on campus is free both days, but fare is still required for any off campus travel.

Shuttle Services

As campus parking is limited, graduates and their guests are encouraged to use the free campus shuttle service to travel between commencement events. Shuttles run throughout campus and are scheduled every 10 minutes. Track the current location of any campus shuttle using the Live Shuttle Tracker.

Accessible Parking

For a map to all accessible parking options on campus, visit the campus map and select the "Accessible" option from the Map Features drop-down menu.

Construction Alerts

For a map with notifications regarding all parking lots effected by campus construction, view the campus map and select the "Construction" option from the Map Features drop-down menu.

Commuter Services

For more information about transportation and parking options, visit the Commuter Services website.

To learn more, please visit the Commencement Ceremony Parking & Transportation page.


March For Science, April 22

Saturday, April 22, 2017 @ 3:00 p.m. - March for Science at City Creek Center

March for Science

Date & Time: Saturday, April 22, 2017 @ 3:00 p.m

Location: City Creek Center
View Map

Click here, or contact the College of Science at (801) 581-6958, to learn more about the March for Science.


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