Research in planetary formation, astrophysics, and cosmology at Bristol
Lead Research Organisation:
University of Bristol
Department Name: Physics
Abstract
This proposal is for a grant to investigate several important questions in planetary science, astrophysics, and cosmology in the Schools of Physics and Earth Sciences in the University of Bristol.
The first project is an investigation of how the Moon formed. The best current idea is that the Moon was created by a giant impact between a massive protoplanet and the young Earth. The problem is that this leads to predictions for the chemical makeup of the Moon that differ from what we measure. Alternative impact scenarios exist, and the key to choosing between them is good measurements of the mix of elements (and different isotopes of those elements) on the Moon. This project will make a far more precise set of measurements of moon rocks than has been possible in the past, with the expectation of being able to choose one model over another.
The second project involves using new data from the Cassini spacecraft to investigate the atmosphere of Saturn's giant moon, Titan. The project will determine how Titan's climate system operates
and how the atmosphere redistributes solar energy over two of Titan's 7.5 Earth-year long seasons. Titan is one of only four terrestrial planets with atmospheres in our Solar System and provides unique
insight into how planetary atmospheres operate under extreme conditions.
The final planetary science project is an investigation of how planets form from the small particles in the gas/dust disks around young stars. We now know that planets are very common around stars, but we are still unsure of how planets form, and even of the best way to search for forming planets within these disks. The purpose of the high-performance computer calculations to be done in this project is to predict where planets can be located in the types of disk that we know exist.
Much cosmology over the past few years has been based on investigations of clusters of galaxies, and the fourth project is to investigate the sample of clusters of galaxies returned by the largest single survey conducted by the XMM-Newton X-ray astronomy satellite. This survey has found thousands of X-ray sources, about 1000 of which are clusters of galaxies which emit X-rays from the hot gas that they contain. This hot-gas emission can be used to estimate the masses of the clusters, and the distribution of cluster masses, which changes over cosmic time, is an excellent test for the type of Universe that we inhabit.
The fifth project investigates one of the issues with understanding the atmospheres of clusters of galaxies - the question of why the radiation from their atmospheres doesn't cause them to cool down, and stop being X-ray sources. The answer seems to be that the gas in clusters is reheated by the ejection of very hot, fast, gas from the regions near black holes at the centres of some of the galaxies in the clusters. This project is aimed at understanding the processes involved in that heating, the physics of the fast gas ejections, and whether the gas coming out from near black holes can make cluster gas magnetic.
While the clusters change with time, because of gas cooling and heating, and the changing size of the Universe, the galaxies within them also change. The sixth project is looking at how the galaxies within clusters change as the clusters change, and how clusters affect galaxies, and galaxies affect clusters. It is now possible to see very young clusters of galaxies, back when the Universe was only about 20% of its current age, and by tracking the changes in the galaxies and clusters from then until the present it may be possible to understand what is going on.
The final project involves the maintenance and improvement of codes used to work with catalogues of astronomical objects. These codes are essential when dealing with modern astronomical data, and are used world-wide, so are of great importance to many astronomers. Some have even found their way into public products like the Microsoft World-Wide Telescope.
The first project is an investigation of how the Moon formed. The best current idea is that the Moon was created by a giant impact between a massive protoplanet and the young Earth. The problem is that this leads to predictions for the chemical makeup of the Moon that differ from what we measure. Alternative impact scenarios exist, and the key to choosing between them is good measurements of the mix of elements (and different isotopes of those elements) on the Moon. This project will make a far more precise set of measurements of moon rocks than has been possible in the past, with the expectation of being able to choose one model over another.
The second project involves using new data from the Cassini spacecraft to investigate the atmosphere of Saturn's giant moon, Titan. The project will determine how Titan's climate system operates
and how the atmosphere redistributes solar energy over two of Titan's 7.5 Earth-year long seasons. Titan is one of only four terrestrial planets with atmospheres in our Solar System and provides unique
insight into how planetary atmospheres operate under extreme conditions.
The final planetary science project is an investigation of how planets form from the small particles in the gas/dust disks around young stars. We now know that planets are very common around stars, but we are still unsure of how planets form, and even of the best way to search for forming planets within these disks. The purpose of the high-performance computer calculations to be done in this project is to predict where planets can be located in the types of disk that we know exist.
Much cosmology over the past few years has been based on investigations of clusters of galaxies, and the fourth project is to investigate the sample of clusters of galaxies returned by the largest single survey conducted by the XMM-Newton X-ray astronomy satellite. This survey has found thousands of X-ray sources, about 1000 of which are clusters of galaxies which emit X-rays from the hot gas that they contain. This hot-gas emission can be used to estimate the masses of the clusters, and the distribution of cluster masses, which changes over cosmic time, is an excellent test for the type of Universe that we inhabit.
The fifth project investigates one of the issues with understanding the atmospheres of clusters of galaxies - the question of why the radiation from their atmospheres doesn't cause them to cool down, and stop being X-ray sources. The answer seems to be that the gas in clusters is reheated by the ejection of very hot, fast, gas from the regions near black holes at the centres of some of the galaxies in the clusters. This project is aimed at understanding the processes involved in that heating, the physics of the fast gas ejections, and whether the gas coming out from near black holes can make cluster gas magnetic.
While the clusters change with time, because of gas cooling and heating, and the changing size of the Universe, the galaxies within them also change. The sixth project is looking at how the galaxies within clusters change as the clusters change, and how clusters affect galaxies, and galaxies affect clusters. It is now possible to see very young clusters of galaxies, back when the Universe was only about 20% of its current age, and by tracking the changes in the galaxies and clusters from then until the present it may be possible to understand what is going on.
The final project involves the maintenance and improvement of codes used to work with catalogues of astronomical objects. These codes are essential when dealing with modern astronomical data, and are used world-wide, so are of great importance to many astronomers. Some have even found their way into public products like the Microsoft World-Wide Telescope.
Planned Impact
Direct beneficiaries from the research will be our academic colleagues and interested members of the public, who will be exposed to the research results through our lectures, talks in schools, podcasts, press releases, WWW pages, appearances on radio and TV, and exhibits in and around Bristol. More indirectly, the public may be affected by advice given to local MPs (Stephen Williams, Liam Fox) or City Councillors (such as Mark Wright, who did a PhD in the Astrophysics Group a few years ago).
Commercial benefits have already been had from the Isotope Group's research (via projects with Shell) and the TOPCAT work (projects with Microsoft Research). Spin-offs from the instrumentation development in the isotope work have benefitted Thermo-Fisher Finnigan, and from the Fourier Transform spectrometer constructed for the radio telescope have benefitted BEAM and AlphaData.
More generically, the sophisticated image and time-series analysis techniques used in our research can be applied to many problems. We will continue to work with the Atomic Force Microscopy group in the University to improve their imaging (as in recent imaging of moving DNA molecules), and are actively exploring the application of our techniques to medical imaging through the Clinical Research and Imaging Centre of the University.
Finally, the major economic output of this work will continue to be trained PhDs and PDRAs who mostly go into non-academic areas for their later careers. These careers have included local Government, the defense and security sector, plasma fusion research, meteorology, teaching, and finance.
Commercial benefits have already been had from the Isotope Group's research (via projects with Shell) and the TOPCAT work (projects with Microsoft Research). Spin-offs from the instrumentation development in the isotope work have benefitted Thermo-Fisher Finnigan, and from the Fourier Transform spectrometer constructed for the radio telescope have benefitted BEAM and AlphaData.
More generically, the sophisticated image and time-series analysis techniques used in our research can be applied to many problems. We will continue to work with the Atomic Force Microscopy group in the University to improve their imaging (as in recent imaging of moving DNA molecules), and are actively exploring the application of our techniques to medical imaging through the Clinical Research and Imaging Centre of the University.
Finally, the major economic output of this work will continue to be trained PhDs and PDRAs who mostly go into non-academic areas for their later careers. These careers have included local Government, the defense and security sector, plasma fusion research, meteorology, teaching, and finance.
Organisations
Publications
Šlaus B
(2020)
The XXL Survey XLI. Radio AGN luminosity functions based on the GMRT 610 MHz continuum observations
in Astronomy & Astrophysics
Zou S
(2016)
The X-ray luminosity-temperature relation of a complete sample of low-mass galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Ziparo F
(2016)
The XXL Survey X. K -band luminosity - weak-lensing mass relation for groups and clusters of galaxies?
in Astronomy & Astrophysics
Zavala J. A.
(2018)
VizieR Online Data Catalog: SCUBA-2 EGS deep field (Zavala+, 2017)
in VizieR Online Data Catalog
Zavala J
(2017)
The SCUBA-2 Cosmology Legacy Survey: the EGS deep field - I. Deep number counts and the redshift distribution of the recovered cosmic infrared background at 450 and 850 µ m
in Monthly Notices of the Royal Astronomical Society
Yuan Z
(2018)
Determining the Core Radio Luminosity Function of Radio AGNs via Copula
in The Astrophysical Journal Supplement Series
Young A.
(2017)
Physically motivated X-ray reverberation models
in From the Dolomites to the Event Horizon: Sledging Down the Black Hole Potential
Young A
(2018)
The absence of a thin disc in M81*
in Monthly Notices of the Royal Astronomical Society
Yao H
(2020)
Galaxy and Mass Assembly (GAMA): A WISE Study of the Activity of Emission-line Systems in G23
in The Astrophysical Journal
Wykes S
(2019)
A 1D fluid model of the Centaurus A jet
in Monthly Notices of the Royal Astronomical Society
Wright A
(2017)
Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function to z = 0.1 from the r-band selected equatorial regions
in Monthly Notices of the Royal Astronomical Society
Worrall Diana
(2017)
The X-ray-radio morphology anomaly in a high-redshift quasar jet
in Chandra Proposal
Worrall Diana
(2016)
Jet-gas interactions and hotspots in FR I/II transition sources
in 41st COSPAR Scientific Assembly
Worrall Diana
(2016)
The interactions of a `switching off' radio galaxy at crucial radio power
in Chandra Proposal
Worrall Diana
(2017)
The X-ray-radio morphology anomaly in a high-redshift quasar jet
in HST Proposal
Worrall D. M.
(2017)
A non cool-core 4.6-keV cluster around the bright nearby radio galaxy PKS B1416-493
in ArXiv e-prints
Worrall D
(2016)
X-rays associated with the jet-cloud-interacting radio galaxy 3C 277.3 (Coma A): implications for energy deposition
in Monthly Notices of the Royal Astronomical Society
Wise Michael W.
(2017)
Deep X-ray Observations of an Ongoing Merger and 400 Myr of AGN Activity in Cygnus A
in AAS/High Energy Astrophysics Division #16
Wise Michael W.
(2017)
Evidence for a TDE Origin for the Radio Transient in Cygnus A
in AAS/High Energy Astrophysics Division #16
West M
(2017)
Ten billion years of brightest cluster galaxy alignments
in Nature Astronomy
West M
(2019)
Publisher Correction: Ten billion years of brightest cluster galaxy alignments
in Nature Astronomy
Wang L
(2018)
GAMA/H-ATLAS: the local dust mass function and cosmic density as a function of galaxy type - a benchmark for models of galaxy evolution
in Monthly Notices of the Royal Astronomical Society
Veras Dimitri
(2017)
Simulating the tidal disruption of the asteroid orbiting white dwarf WD 1145+017
in AAS/Division of Dynamical Astronomy Meeting #48
Veras D.
(2017)
Constraining properties of disintegrating exoplanets
in European Planetary Science Congress
Veras D
(2017)
Explaining the variability of WD 1145+017 with simulations of asteroid tidal disruption
in Monthly Notices of the Royal Astronomical Society
Van Der Burg R
(2017)
The abundance of ultra-diffuse galaxies from groups to clusters UDGs are relatively more common in more massive haloes
in Astronomy & Astrophysics
Tremblay GR
(2016)
Cold, clumpy accretion onto an active supermassive black hole.
in Nature
Tremblay G
(2015)
Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies
in Monthly Notices of the Royal Astronomical Society
Tremblay G
(2018)
A Galaxy-scale Fountain of Cold Molecular Gas Pumped by a Black Hole
in The Astrophysical Journal
Teuben Peter
(2016)
Implementing Ideas for Improving Software Citation and Credit
in arXiv e-prints
Taylor Mark
(2017)
TOPCAT: Desktop Exploration of Tabular Data for Astronomy and Beyond
in arXiv e-prints
Taylor Mark
(2017)
TOPCAT: Working with Data and Working with Users
in arXiv e-prints
Taylor Mark
(2018)
TOPCAT and Gaia
in arXiv e-prints
Taylor Mark
(2015)
TOPCAT's TAP Client
in arXiv e-prints
Taylor M. B.
(2015)
External Use of TOPCAT's Plotting Library
in Astronomical Data Analysis Software an Systems XXIV (ADASS XXIV)
Taylor M. B.
(2017)
TOPCAT's TAP Client
in Astronomical Data Analysis Software and Systems XXV
Taylor M. B.
(2016)
All of the Sky: HEALPix Density Maps of Gaia-scale Datasets from the Database to the Desktop
in arXiv e-prints
Taylor M
(2015)
SAMP, the Simple Application Messaging Protocol: Letting applications talk to each other
in Astronomy and Computing
Taylor E
(2020)
GAMA + KiDS: empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
in Monthly Notices of the Royal Astronomical Society
Tanvir N. R.
(2017)
The properties of GRB 120923A at a spectroscopic redshift of z=7.8
in ArXiv e-prints
Tanvir N
(2018)
The Properties of GRB 120923A at a Spectroscopic Redshift of z ˜ 7.8
in The Astrophysical Journal
Sánchez-Portal M
(2015)
GLACE survey: OSIRIS/GTC tuneable filter H a imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395 I. Survey presentation, TF data reduction techniques, and catalogue?
in Astronomy & Astrophysics
Su K. Y. L.
(2019)
VizieR Online Data Catalog: IRAC fluxes of the ID8 and P1121 systems (Su+, 2019)
in VizieR Online Data Catalog
Su K
(2019)
Extreme Debris Disk Variability: Exploring the Diverse Outcomes of Large Asteroid Impacts During the Era of Terrestrial Planet Formation
in The Astronomical Journal
Stewart S. T.
(2016)
Mercury Impact Origin Hypothesis Survives the Volatile Crisis: Implications for Terrestrial Planet Formation
in 47th Annual Lunar and Planetary Science Conference
Snios Bradford
(2018)
The Cocoon Shocks of Cygnus A: Pressures and Their Implications for the Jets and Lobes
in ArXiv e-prints
Snios Bradford
(2019)
Variability and Proper Motion of X-ray Knots in the Jet of Centaurus A
in American Astronomical Society Meeting Abstracts #233
Snios B
(2018)
The Cocoon Shocks of Cygnus A: Pressures and Their Implications for the Jets and Lobes
in The Astrophysical Journal
Smolcic V
(2018)
The XXL Survey XXIX. GMRT 610 MHz continuum observations
in Astronomy & Astrophysics
Smolcic V
(2016)
The XXL Survey XI. ATCA 2.1 GHz continuum observations?
in Astronomy & Astrophysics
Description | The properties of quasar jets have been shown to be incompatible with the standard model for their origin. The evolution of galaxies through the "green valley" has been exposed. Survey work on X-ray clusters of galaxies is yielding cosmological and astrophysical results through a long series of publications. Work on the sub-mm and IR properties of early galaxies has been advanced, again through surveys, but also through gravitational lensing investigations. Software developments are commercially useful and are being applied by partners. |
Exploitation Route | The astrophysical results will lead to further investigations in a number of areas. |
Sectors | Education,Culture, Heritage, Museums and Collections,Transport |
Description | STFC Impact Accelerator Account |
Amount | £15,793 (GBP) |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 03/2015 |
End | 12/2015 |
Description | STFC Impact Accelerator Account |
Amount | £20,302 (GBP) |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 07/2014 |
End | 06/2015 |
Title | TOPCAT |
Description | TOPCAT is the most-used astronomical catalogue handling tool. It is extensively used to handle Gaia data and to create exploration plots of stellar populations, as well as in many other astronomical applications. It is also used for education in astronomical methods in the UK, Africa, and elsewhere. The underlying libraries are also used extensively for software developments. |
Type Of Material | Improvements to research infrastructure |
Provided To Others? | Yes |
Impact | Extensively used world-wide. |
URL | http://www.star.bris.ac.uk/~mbt/topcat/ |
Title | STILTS |
Description | Starlink Tables Infrastructure Library Tool Set: software for handling tabular data in many formats, including methods compliant with Virtual Observatory protocols. |
Type Of Material | Data handling & control |
Year Produced | 2010 |
Provided To Others? | No |
Impact | Used in many astronomical databases; potential uses for other complicated databases. |
Title | TOPCAT |
Description | Tool for operations on catalogues and tables: general catalogue comparison/selection tool, much used by astronomers world-wide. |
Type Of Material | Data handling & control |
Year Produced | 2011 |
Provided To Others? | No |
Impact | Extensible to many table-based datasets where matching of entries is required. Has been used on experimental basis for medical work, for example. |
Title | STILTS |
Description | Set of command-line tools that can be used for powerful astronomical catalogue interrogation, manipulation, and plotting. 2010 releases v2.1-2, v2.2, v2.2-1 2011 releases v2.3, v2.3-1, v2.4 2013 releases v2.5, v2.5-1, v2.5-2 2014 releases v2.5-3, v3.0 |
Type Of Technology | Software |
Year Produced | 2010 |
Open Source License? | Yes |
Impact | Heavily used in catalogue manipulation, world-wide. |
URL | http://www.starlink.ac.uk/stilts/ |
Title | TOPCAT |
Description | Astronomical data-handling software |
Type Of Technology | Software |
Year Produced | 2010 |
Open Source License? | Yes |
Impact | Used internationally for interaction with large distributed databases. 2010 releases v3.5-2, v3.6, v3.7 2011 releases v3.8, v3.9 2013 releases v4.0b, v4.0-1 2014 releases v4.1, v4.2 |
URL | http://www.starlink.ac.uk/topcat/ |
Description | Development of grant with "We the Curious", Bristol |
Form Of Engagement Activity | A formal working group, expert panel or dialogue |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Other audiences |
Results and Impact | Development of proposal for engagement with individuals with visual impairment - so they can participate in astronomy. |
Year(s) Of Engagement Activity | 2017,2018 |
Description | Public lectures and science cafes |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Multiple public talks to astronomy societies and other organisations, also Science Cafes and other groups (e.g., Anglo-Polish society). Activities tended to go on to time limit because of question-and-answer sessions, and have generated eMail questions after the fact from attendees. Continued requests for talks and other contacts based on experiences. |
Year(s) Of Engagement Activity | 2006,2007,2008,2009,2010,2011,2012,2013,2014 |
Description | Radio interview (BBC Radio Bristol; BBC Radio 4; BBC Radio Scotland) |
Form Of Engagement Activity | A press release, press conference or response to a media enquiry/interview |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Media (as a channel to the public) |
Results and Impact | Contacts from regional amateur astronomers, and astronomical societies. Talks to local societies. |
Year(s) Of Engagement Activity | 2012,2013,2014 |
Description | School student placements |
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 | Schools |
Results and Impact | 1/2 students per year visited the Group and worked with staff Students became more focussed in aims for science sstudies at University level. |
Year(s) Of Engagement Activity | 2012,2013,2014 |