Queen's University Belfast Astronomy Observation and Theory Consolidated Grant 2020-2023
Lead Research Organisation:
Queen's University Belfast
Department Name: Sch of Mathematics and Physics
Abstract
Supernovae create the heavy chemical elements we see in our solar system, the Galaxy and entire visible Universe. While stars evolve over millions or billions of years, a supernova explosion happens in seconds and the glowing remnant lasts for years. We aim to understand how these explosions happen and how they create the neutron stars, pulsars and black holes in our galaxy. In 2017 a breakthrough discovery was made when the first electromagnetic counterpart to a gravitational wave source was found. This was termed a kilonova because it was 1000 times brighter than a nova. The gravitational waves and the kilonova were from a pair of merging neutron stars. The optical and infrared light arose from the radioactive decay of heavy elements, which we call r-process elements. These are heavier than iron in the periodic table and such neutron star mergers may be responsible for all these heavy elements. Or projects will find more of these in the coming years and the combination of gravitational waves and electromagnetic signals opens up a new window on the Universe.
The thermonuclear supernovae that are used as cosmic yardsticks and led to the Nobel Prize winning discovery of dark energy come from white dwarf stars. But exactly how they explode and what the progenitor systems are still eludes us. A white dwarf is a star greater than the mass of the sun, but the size of the earth. They are incredibly dense, one teaspoon of WD material weighs about 10 thousand tonnes. To understand how they explode, we will model their spectra with the most sophisticated 3 dimensional computer models that currently exist.
The elements created in supernovae form planetary systems in our galaxy - iron, silicon, oxygen, magnesium are all critical to forming planetary systems. The diversity in the known planetary systems around other stars in our galaxy (called exoplanets) is astounding. We know of thousands of exoplanets. Hot Jupiters, multiple planetary systems and super-earths are now commonly found in surveys to discover new planets. We can see planet formation in the disks of young stars during their first few million years of life. The latest large facility built in the southern hemisphere (ALMA), has provided spectacular data on proto-planetary disks and our work on the chemistry of the disk aims to understand their origins. Our top priority in this area is to find another earth like planet - the right size, age and distance from its parent star to support an atmosphere and liquid water. This search requires careful tests of the methods to extract the tiny signals we expect and we propose to develop this with an eye on the future prize of detecting an earth twin. We will soon have extraordinarily precise spectrometers on the biggest telescopes to measure the velocity of stars down to metres per second. At this level, it is no longer the instrument measuring precision that hinders our planet searching, but the real activity on the surface of Sun like stars. Our project will aim to understand and mitigate this effect.
A critical part of astrophysics is pulling together our detailed knowledge of physics that we can measure on earth to what we can only see (through electromagnetic radiation) in the distant Universe. This will be done through computer calculations of model atoms. These codes calculate how electrons are excited in atoms and ensures that astrophysical models identify the elements that cause the spectral lines in supernovae, supermassive black holes, galaxy spectra and stars. Now that we have detected a kilonova we must do the same calculations for the heaviest elements.
We will also run novel experiments to use powerful lasers (e.g. the VULCAN laser) to mimic the physics of gas that causes x-ray emission in accreting sources such as black hole binaries. We will use these novel laboratory data to test the world's leading computer code that is used to model the central regions of galaxies close to their black holes.
The thermonuclear supernovae that are used as cosmic yardsticks and led to the Nobel Prize winning discovery of dark energy come from white dwarf stars. But exactly how they explode and what the progenitor systems are still eludes us. A white dwarf is a star greater than the mass of the sun, but the size of the earth. They are incredibly dense, one teaspoon of WD material weighs about 10 thousand tonnes. To understand how they explode, we will model their spectra with the most sophisticated 3 dimensional computer models that currently exist.
The elements created in supernovae form planetary systems in our galaxy - iron, silicon, oxygen, magnesium are all critical to forming planetary systems. The diversity in the known planetary systems around other stars in our galaxy (called exoplanets) is astounding. We know of thousands of exoplanets. Hot Jupiters, multiple planetary systems and super-earths are now commonly found in surveys to discover new planets. We can see planet formation in the disks of young stars during their first few million years of life. The latest large facility built in the southern hemisphere (ALMA), has provided spectacular data on proto-planetary disks and our work on the chemistry of the disk aims to understand their origins. Our top priority in this area is to find another earth like planet - the right size, age and distance from its parent star to support an atmosphere and liquid water. This search requires careful tests of the methods to extract the tiny signals we expect and we propose to develop this with an eye on the future prize of detecting an earth twin. We will soon have extraordinarily precise spectrometers on the biggest telescopes to measure the velocity of stars down to metres per second. At this level, it is no longer the instrument measuring precision that hinders our planet searching, but the real activity on the surface of Sun like stars. Our project will aim to understand and mitigate this effect.
A critical part of astrophysics is pulling together our detailed knowledge of physics that we can measure on earth to what we can only see (through electromagnetic radiation) in the distant Universe. This will be done through computer calculations of model atoms. These codes calculate how electrons are excited in atoms and ensures that astrophysical models identify the elements that cause the spectral lines in supernovae, supermassive black holes, galaxy spectra and stars. Now that we have detected a kilonova we must do the same calculations for the heaviest elements.
We will also run novel experiments to use powerful lasers (e.g. the VULCAN laser) to mimic the physics of gas that causes x-ray emission in accreting sources such as black hole binaries. We will use these novel laboratory data to test the world's leading computer code that is used to model the central regions of galaxies close to their black holes.
Planned Impact
We have an active and energetic outreach and engagement programme to target audiences locally in Northern Ireland and nationally in the UK. We have had major success in publicising our research in the media, from local radio and newspapers through to national TV appearances. Highlights of our UK national media presence are appearances on BBC, Channel 4, RTE (Republic of Ireland National broadcaster), as part of the world-wide press on the electromagnetic counterpart to a gravitational wave source. We were invited to make the public announcement of the discovery at the world-wide ESO press conference in Munich in October 2017.
We have been invited to talk at the British Science Festival (2018) and the Northern Ireland Science Festival (2017). To increase the public awareness of science in Northern Ireland we have made a focused effort to engage with the local media (BBC and independent broadcasters) to showcase our research highlights and related public events. Over the last 4-5 years, astronomers from Astrophysics Research Centre have had over 40 appearances on BBC Northern Ireland (radio and TV), RTE, or other regional broadcasts or in mainstream UK newspapers. These include the premier local radio shows - BBC Radio Ulster "Good Morning Ulster" and "Evening Extra" and the BBC NI Newsline (the main 6:30pm TV news show). These are the primary BBC news and magazine shows in the weekday morning and evenings, with typical listening figures of 295,000 for the morning and evening radio shows and 140,000 for TV.
We host, support and sponsor bi-monthly meetings of the Irish Astronomical Association (IAA) at Queen's which brings in around 80 people each meeting. ARC staff regularly give lectures and use our influence to bring in speakers from Britain and Europe
We regularly support initiatives by local astronomy societies. This has included opening exhibitions of astronomical photographs (in the Carnegie Library in County Down) and running a selection of the best astronomical image in the "Heaven's Above" exhibition. The winner is currently being made into a large scale artwork to be displayed in the Main Physics Building at Queen's.
We regularly deliver astronomy lectures and presentations at the following annual events: (i) QUB Horizons in Physics (which attracts around 400 Year 11-12 students per annum), (ii) Physics Open Days (around 200 Y13 students), (iii) Physics Teachers Conference (about 50 Physics teachers from schools in Ireland).
We have frequent and regular requests to talk at Science Cafés - with one of the most popular being the "Science of Science Fiction talks" delivered by Keenan.
Between 2010-2017 (covering the previous consolidated grant period) the application rate to physics based courses in QUB increased by 80%, and we have maintained that application rate in the last two years. This coincided with our focused and energetic outreach efforts in Schools, museums, and public outreach events.
We worked with the Zooniverse project to add Pan-STARRS data to the Supernova Hunters project : this had huge take up, with the citizen scientists being able to find real supernovae and turn around 1000s of candidate images per day. This also led to a comparison between our Machine Learning and human classifiers (Wright et al. 2017, MNRAS, 472, 1315). For 2019, we are in discussions with an Ireland-wide Physics consortium to bring the IAU "Above and Beyond" exhibition on a tour of the island. This exhibition has been commissioned to coincide with the IAU 100th Anniversary celebrations.
We have engaged with 2 UK companies (Andor and E2V/Teledyne) to purchase detectors and cameras for the SOXS system and also have acted as advisors to Andor on the application and commercialisation of InGaAS arrays in astronomy.
We have been invited to talk at the British Science Festival (2018) and the Northern Ireland Science Festival (2017). To increase the public awareness of science in Northern Ireland we have made a focused effort to engage with the local media (BBC and independent broadcasters) to showcase our research highlights and related public events. Over the last 4-5 years, astronomers from Astrophysics Research Centre have had over 40 appearances on BBC Northern Ireland (radio and TV), RTE, or other regional broadcasts or in mainstream UK newspapers. These include the premier local radio shows - BBC Radio Ulster "Good Morning Ulster" and "Evening Extra" and the BBC NI Newsline (the main 6:30pm TV news show). These are the primary BBC news and magazine shows in the weekday morning and evenings, with typical listening figures of 295,000 for the morning and evening radio shows and 140,000 for TV.
We host, support and sponsor bi-monthly meetings of the Irish Astronomical Association (IAA) at Queen's which brings in around 80 people each meeting. ARC staff regularly give lectures and use our influence to bring in speakers from Britain and Europe
We regularly support initiatives by local astronomy societies. This has included opening exhibitions of astronomical photographs (in the Carnegie Library in County Down) and running a selection of the best astronomical image in the "Heaven's Above" exhibition. The winner is currently being made into a large scale artwork to be displayed in the Main Physics Building at Queen's.
We regularly deliver astronomy lectures and presentations at the following annual events: (i) QUB Horizons in Physics (which attracts around 400 Year 11-12 students per annum), (ii) Physics Open Days (around 200 Y13 students), (iii) Physics Teachers Conference (about 50 Physics teachers from schools in Ireland).
We have frequent and regular requests to talk at Science Cafés - with one of the most popular being the "Science of Science Fiction talks" delivered by Keenan.
Between 2010-2017 (covering the previous consolidated grant period) the application rate to physics based courses in QUB increased by 80%, and we have maintained that application rate in the last two years. This coincided with our focused and energetic outreach efforts in Schools, museums, and public outreach events.
We worked with the Zooniverse project to add Pan-STARRS data to the Supernova Hunters project : this had huge take up, with the citizen scientists being able to find real supernovae and turn around 1000s of candidate images per day. This also led to a comparison between our Machine Learning and human classifiers (Wright et al. 2017, MNRAS, 472, 1315). For 2019, we are in discussions with an Ireland-wide Physics consortium to bring the IAU "Above and Beyond" exhibition on a tour of the island. This exhibition has been commissioned to coincide with the IAU 100th Anniversary celebrations.
We have engaged with 2 UK companies (Andor and E2V/Teledyne) to purchase detectors and cameras for the SOXS system and also have acted as advisors to Andor on the application and commercialisation of InGaAS arrays in astronomy.
Organisations
Publications
Eappachen D
(2024)
XMM- Newton -discovered Fast X-ray Transients: host galaxies and limits on contemporaneous detections of optical counterparts
in Monthly Notices of the Royal Astronomical Society
Eappachen D
(2024)
XMM- Newton -discovered Fast X-ray Transients: host galaxies and limits on contemporaneous detections of optical counterparts
in Monthly Notices of the Royal Astronomical Society
Bulla M
(2020)
White dwarf deflagrations for Type Iax supernovae: polarisation signatures from the explosion and companion interaction
in Astronomy & Astrophysics
Acharyya A
(2023)
VERITAS Discovery of Very High Energy Gamma-Ray Emission from S3 1227+25 and Multiwavelength Observations
in The Astrophysical Journal
Lawson K
(2021)
Use of the Culham He model He II atomic data in JET EDGE2D-EIRENE simulations
in Nuclear Materials and Energy
Lienhard F
(2023)
Unsigned magnetic flux proxy from solar optical intensity spectra
in Monthly Notices of the Royal Astronomical Society
Srivastav S
(2023)
Unprecedented Early Flux Excess in the Hybrid 02es-like Type Ia Supernova 2022ywc Indicates Interaction with Circumstellar Material
in The Astrophysical Journal Letters
Srivastav S
(2023)
Unprecedented Early Flux Excess in the Hybrid 02es-like Type Ia Supernova 2022ywc Indicates Interaction with Circumstellar Material
in The Astrophysical Journal Letters
Lach F
(2022)
Type Iax supernovae from deflagrations in Chandrasekhar mass white dwarfs
in Astronomy & Astrophysics
Spyratos P
(2021)
Transmission spectroscopy with VLT FORS2: a featureless spectrum for the low-density transiting exoplanet WASP-88b
in Monthly Notices of the Royal Astronomical Society
Cherubim C
(2023)
TOI-1695 b: A Water World Orbiting an Early-M Dwarf in the Planet Radius Valley
in The Astronomical Journal
Cloutier R
(2021)
TOI-1634 b: An Ultra-short-period Keystone Planet Sitting inside the M-dwarf Radius Valley
in The Astronomical Journal
Johnson C
(2023)
Time-dependent collisional radiative modeling of tungsten in the magnetic sheath for erosion diagnosis
in Nuclear Fusion
Yao Y
(2023)
Tidal Disruption Event Demographics with the Zwicky Transient Facility: Volumetric Rates, Luminosity Function, and Implications for the Local Black Hole Mass Function
in The Astrophysical Journal Letters
Gill S
(2022)
TIC-320687387 B: a long-period eclipsing M-dwarf close to the hydrogen burning limit
in Monthly Notices of the Royal Astronomical Society
Psaridi A
(2023)
Three Saturn-mass planets transiting F-type stars revealed with TESS and HARPS TOI-615b, TOI-622b, and TOI-2641b
in Astronomy & Astrophysics
Sollerman J
(2021)
Three Core-Collapse Supernovae with Nebular Hydrogen Emission
Kenworthy M
(2021)
The ß Pictoris b Hill sphere transit campaign I. Photometric limits to dust and rings
in Astronomy & Astrophysics
Jones D
(2021)
The Young Supernova Experiment: Survey Goals, Overview, and Operations
in The Astrophysical Journal
Aleo P
(2023)
The Young Supernova Experiment Data Release 1 (YSE DR1): Light Curves and Photometric Classification of 1975 Supernovae
in The Astrophysical Journal Supplement Series
Barragán O
(2022)
The young HD 73583 (TOI-560) planetary system: two 10-M? mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf
in Monthly Notices of the Royal Astronomical Society
Yao Y
(2022)
The X-Ray and Radio Loud Fast Blue Optical Transient AT2020mrf: Implications for an Emerging Class of Engine-driven Massive Star Explosions
in The Astrophysical Journal
Montargès M
(2023)
The VLT/SPHERE view of the ATOMIUM cool evolved star sample I. Overview: Sample characterization through polarization analysis
in Astronomy & Astrophysics
Lennon D
(2022)
The VLT-FLAMES survey of massive stars NGC 2004#115: A triple system hosting a possible short period B+BH binary
in Astronomy & Astrophysics
Millar T
(2024)
The UMIST Database for Astrochemistry 2022
in Astronomy & Astrophysics
Sollerman J
(2021)
The Type II supernova SN 2020jfo in M 61, implications for progenitor system, and explosion dynamics
in Astronomy & Astrophysics
Ben-Ami T
(2023)
The Type Ibn Supernova 2019kbj: Indications for Diversity in Type Ibn Supernova Progenitors
in The Astrophysical Journal
Petrushevska T
(2023)
The rise and fall of the iron-strong nuclear transient PS16dtm
in Astronomy & Astrophysics
Fulton M
(2023)
The Optical Light Curve of GRB 221009A: The Afterglow and the Emerging Supernova
in The Astrophysical Journal Letters
Onori F
(2022)
The nuclear transient AT 2017gge: a tidal disruption event in a dusty and gas-rich environment and the awakening of a dormant SMBH
in Monthly Notices of the Royal Astronomical Society
Srivastav S
(2022)
The luminous type Ia supernova 2022ilv and its early excess emission
Srivastav S
(2023)
The Luminous Type Ia Supernova 2022ilv and Its Early Excess Emission
in The Astrophysical Journal Letters
Srivastav S
(2020)
The Lowest of the Low: Discovery of SN 2019gsc and the Nature of Faint Iax Supernovae
in The Astrophysical Journal Letters
Van De Sande M
(2022)
The impact of UV photons from a stellar companion on the chemistry of AGB outflows
in Proceedings of the International Astronomical Union
Van de Sande M
(2022)
The impact of stellar companion UV photons on the chemistry of the circumstellar environments of AGB stars
in Monthly Notices of the Royal Astronomical Society
Nagy Z
(2023)
The Gaia alerted fading of the FUor-type star Gaia21elv
in Monthly Notices of the Royal Astronomical Society
Gutiérrez C
(2021)
The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object
in Monthly Notices of the Royal Astronomical Society
Jackson D
(2023)
The discovery of three hot Jupiters, NGTS-23b, 24b, and 25b, and updated parameters for HATS-54b from the Next Generation Transit Survey
in Monthly Notices of the Royal Astronomical Society
Title | The science of superheroes |
Description | A presentation on the science of superheroes, which contains clips of TV shows and films with superheroes in them (Superman, Avengers etc), along with slides discussing the accuracy or otherwise of the 'science' in the clips. |
Type Of Art | Film/Video/Animation |
Year Produced | 2022 |
Impact | None to date as the presentation has just been completed, and delivery of the presentation is still on hold due to the Covid-19 pandemic. However once it can be given to audiences (ranging from schoolchildren to the general public, teachers, university students etc), it is envisaged that it will be very popular, similar to the previous presentations on the science of science-fiction films and TV shows. |
Description | Chemistry as a tool to study star death |
Amount | £13,152 (GBP) |
Funding ID | EM-2021-069/4 |
Organisation | The Leverhulme Trust |
Sector | Charity/Non Profit |
Country | United Kingdom |
Start | 09/2021 |
End | 03/2023 |
Description | Leverhulme Interdisciplinary Network on Algorithmic Solutions (LINAS) |
Amount | £1,350,000 (GBP) |
Funding ID | 95191 |
Organisation | The Leverhulme Trust |
Sector | Charity/Non Profit |
Country | United Kingdom |
Start | 10/2021 |
End | 08/2025 |
Description | New generation sky surveys, exotic transients and gravitational wave sources |
Amount | £130,337 (GBP) |
Funding ID | ST/X006506/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 04/2023 |
End | 03/2024 |
Description | Queen's University Belfast Astronomy Observation and Theory Consolidated Grant 2023-2026 |
Amount | £1,134,350 (GBP) |
Funding ID | ST/X00094X/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 04/2023 |
End | 03/2026 |
Description | STFC Belfast 2021 DTP |
Amount | £159,496 (GBP) |
Funding ID | ST/W507751/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 09/2021 |
End | 09/2025 |
Description | STFC Belfast 2022 DTP |
Amount | £81,631 (GBP) |
Funding ID | ST/X508706/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 09/2022 |
End | 09/2026 |
Description | Astronomy Open Day for Northern Ireland Science Festival |
Form Of Engagement Activity | Participation in an open day or visit at my research institution |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | An Open Day where members of the public visited the astrophysicists at Queen's University to learn about the latest discoveries and also gain some general knowledge of astronomy. |
Year(s) Of Engagement Activity | 2023 |
Description | Our Place in Space |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Public/other audiences |
Results and Impact | Centered around an epic (and accurate) scale model of the solar system designed by the artist Oliver Jeffers with scientist Professor Stephen Smartt and a creative team led by Nerve Centre, Our Place in Space is a sculpture trail of our solar system, interactive AR app and exciting learning and events programme. In 2022, the Our Place in Space sculpture trail landed on the banks of the River Foyle in Derry (22 April - 22 May) before moving to Divis and the Black Mountain in Belfast (11 June - 10 July). We then travelled across the Irish Sea to Cambridge (30 July - 28 August) followed by Liverpool (14 October - 6 November). The trail returned Northern Ireland at the Ulster Transport Museum and North Down Coastal Path on 24 February - 26 March 2023. Following this, The Sun to Mars will remain on the grounds of the Ulster Transport Museum as a temporary exhibit. We have reached audiences in the few hundred thousands - schools, families, general public. |
Year(s) Of Engagement Activity | 2022,2023 |
URL | https://ourplaceinspace.earth |