- Home
- Search
- Astronomy and Space Science
- Queen Mary University of London
- PhD Astronomy- Planet Formation and Evolution
Course options
-
Qualification
PhD/DPhil - Doctor of Philosophy
-
Location
Main Site
-
Study mode
Full time
-
Start date
SEP
-
Duration
3 Years
Course summary
In the last 15 years over 4000 planets have been discovered around stars other than the Sun. We are now moving beyond just detecting planets, to really understanding their properties and characterising them. It is now clear that planets have very diverse features and to explain this we have to learn how they are formed from flattened "protoplanetary discs’’ of material around young stars, as well as how the planets subsequently evolve. Of course, we ultimately want to understand our own Solar system, and how it fits into the spectrum of planetary architectures.The Planet formation and evolution group at Queen Mary is involved in world leading theoretical and observational research in planet formation and evolution, both within our own Solar system and beyond. We are involved in the Red Dots program, which has resulted in the detection of planets around some of the closest stars to the Sun, including Proxima Centauri, Barnard’s Star and Gliese 887.The Planet formation and evolution group at Queen Mary is involved in world leading theoretical and observational research in planet formation and evolution, both within our own Solar system and beyond. We are involved in the Red Dots program, which has resulted in the detection of planets around some of the closest stars to the Sun, including Proxima Centauri, Barnard’s Star and Gliese 887.Our group also studies the key role that planetary dynamics and collisions play in determining how planets and their satellites form and evolve, with a focus on Solar system planets and moons. The Solar System Dynamics group at Queen Mary was heavily involved in the Cassini mission to Saturn and was directly responsible for the discovery of two new Saturnian moons. The main research interests are the dynamics of planetary rings and their gravitational interaction with small moons orbiting nearby. Understanding these processes has direct applications to the behaviour of evolving protoplanets in a disc. The group also analyses Cassini images to make astrometric measurements of the positions of objects against background stars and thereby detect subtle changes in their orbits over time. This work contributed to new research showing that Saturn’s largest moon Titan was once much closer to the planet.
Tuition fees
- United States
- Afghanistan
- Albania
- Algeria
- Andorra
- Angola
- Antigua & Barbuda
- Argentina
- Armenia
- Australia
- Austria
- Azerbaijan
- Bahamas
- Bahrain
- Bangladesh
- Barbados
- Belarus
- Belgium
- Belize
- Benin
- Bhutan
- Bolivia
- Bosnia and Herzegovina
- Botswana
- Brazil
- Brunei
- Bulgaria
- Burkina Faso
- Burma
- Burundi
- Cabo Verde
- Cambodia
- Cameroon
- Canada
- Central African Republic
- Chad
- Chile
- China
- Colombia
- Comoros
- Congo
- Congo (Democratic Republic)
- Costa Rica
- Croatia
- Cuba
- Curacao
- Cyprus
- Czech Republic
- Denmark
- Djibouti
- Dominica
- Dominican Republic
- East Timor
- Ecuador
- Egypt
- El Salvador
- England
- Equatorial Guinea
- Eritrea
- Estonia
- Ethiopia
- Fiji
- Finland
- France
- Gabon
- Gambia
- Georgia
- Germany
- Ghana
- Greece
- Grenada
- Guatemala
- Guinea
- Guinea-Bissau
- Guyana
- Haiti
- Honduras
- Hong Kong
- Hungary
- Iceland
- India
- Indonesia
- Iran
- Iraq
- Israel
- Italy
- Ivory Coast
- Jamaica
- Japan
- Jordan
- Kazakhstan
- Kenya
- Kiribati
- Korea DPR (North Korea)
- Kosovo
- Kuwait
- Kyrgyzstan
- Laos
- Latvia
- Lebanon
- Lesotho
- Liberia
- Libya
- Liechtenstein
- Lithuania
- Luxembourg
- Macedonia
- Madagascar
- Malawi
- Malaysia
- Maldives
- Mali
- Malta
- Marshall Islands
- Mauritania
- Mauritius
- Mexico
- Micronesia
- Moldova
- Monaco
- Mongolia
- Montenegro
- Morocco
- Mozambique
- Namibia
- Nauru
- Nepal
- Netherlands
- New Zealand
- Nicaragua
- Niger
- Nigeria
- Northern Ireland
- Norway
- Oman
- Pakistan
- Palau
- Palestinian Authority
- Panama
- Papua New Guinea
- Paraguay
- Peru
- Philippines
- Poland
- Portugal
- Puerto Rico
- Qatar
- Republic of Ireland
- Romania
- Russia
- Rwanda
- San Marino
- Sao Tome and Principe
- Saudi Arabia
- Scotland
- Senegal
- Serbia
- Seychelles
- Sierra Leone
- Singapore
- Slovakia
- Slovenia
- Solomon Islands
- Somalia
- South Africa
- South Korea
- South Sudan
- Spain
- Sri Lanka
- St Vincent
- St. Kitts & Nevis
- St. Lucia
- Sudan
- Suriname
- Swaziland
- Sweden
- Switzerland
- Syria
- Taiwan
- Tajikistan
- Tanzania
- Thailand
- Togo
- Tonga
- Trinidad & Tobago
- Tunisia
- Turkey
- Turkmenistan
- Tuvalu
- UAE
- Uganda
- Ukraine
- United Kingdom
- Uruguay
- Uzbekistan
- Vanuatu
- Vatican City
- Venezuela
- Vietnam
- Wales
- Western Samoa
- Yemen
- Zambia
- Zimbabwe
£ 28,850per year
Tuition fees shown are for indicative purposes and may vary. Please check with the institution for most up to date details.
University information
-
University League Table
41st
-
Campus address
Queen Mary University of London, Mile End Road, London, Tower Hamlets, E1 4NS, United Kingdom
Subject rankings
-
Subject ranking
30th out of 91 2
36th out of 48 5
-
Entry standards
/ Max 218143 66%36th
-
Graduate prospects
/ Max 10080.0 80%28th
24 -
Student satisfaction
/ Max 43.02 76%65th
13 -
Entry standards
/ Max 224148 66%31st
-
Graduate prospects
/ Max 10078.0 78%39th
6 -
Student satisfaction
/ Max 43.08 77%35th
3