Dr Raphaëlle D. Haywood
Lecturer in Physics & Astronomy
My research focuses on the detection and characterisation of small, potentially terrestrial planets around other starsthan our Sun (which are known as exoplanets).
I spent most of my childhood in France, then moved to the UK to study Physics and Astrophysics.I obtained my PhD in 2015 at the University of St Andrews, UK.After my PhD, I was a postdoctoral researcher and a NASA Sagan Fellow at Harvard College Observatory, USA.
Leia este artigo da Cientistas Feministas escrito por Meghie Rodrigues para saber mais sobre mim e minha pesquisa!
Funded opportunities to join my research group:I am currently advertising a PhD studentship on Discovering other Earths while sustaining our unique home in the Cosmos,fully funded by the China Scholarship Council in partnership with the University of Exeter.If my research detailed below is of interest to you, then please get in touch with me! Deadline for applications is 11 January 2021.Full details on eligibility and how to apply can be found here.
I will be recruiting a postdoc (3 years) in early 2021, to start in April 2021 or soon thereafter.The postdoc will develop stellar models of radial-velocity variations informed by solar observations and knowledge, and willdetermine precise masses of small planets. Details on how to apply will be posted soon!
About my research:Detecting terrestrial planets is a crucial step to answering some of humanity’s most fundamental questions: What kinds of planets are habitable? Is there life on other planets? How do these findings frame environmental challenges on Earth?
The most viable technique to discover other planets with similar observable properties to Earth is to monitor stars nightly over several years to look for the tiny wobbling induced by planets orbiting it (i.e. monitoring a star's radial velocity). For the first time in human history, we have the technological capability to detect temperate, terrestrial planets orbiting other stars, notably via the Terra Hunting Experiment, which is scheduled to start in 2022.
In my research, I aim to overcome the biggest remaining obstacle: "noise" arising from the intrinsic variability of the host stars themselves.Stellar "noise" also prevents us from determining the masses of exoplanets. Determining robust planetary masses is key to the success of the James Webb Space Telescope, a mission launching in 2021 to observe the atmospheres of exoplanets. These observations, too, will be contaminated by the host stars' intrinsic variability (e.g. see this short conference proceeding by Rackham et al., 2019).
Observing the Sun as an exoplanet-host star:The Sun is the only star whose surface we can image directly and at high resolution; therefore, it is a unique benchmark to explore the physical phenomena responsible for radial-velocity "noise".
Since 2015, we have been observing the Sun as if it were a distant, point-like star, using the exoplanet-hunting spectrograph HARPS-N.
Prior to these observations and during my PhD, my collaborators and I used observations of the Sun (our best-known star) to explore the physical processesresponsible for radial-velocity variations induced by the magnetic activity of the host stars. You can find out more in this UK Solar Physics nugget: The Sun as an Exoplanet Host Star.
I study velocity flows and small-scale magnetic fields on the Sun's surface, that produce radial-velocity signals modulated by the Sun's rotation. With this solar knowledge, I am developing new analysis techniques for exoplanet radial-velocity observations, in order to determine precise and accurate masses of small planets in the presence of stellar variability.I talked about the impact of stellar magnetic activity in exoplanet searches in this Exocast.
Determining the masses of exoplanets in the presence of stellar "noise":In this Astrobites blog post, written by Ben Montet, explains the new analysis technique that I developed in my PhD to determinereliable masses for the planets orbiting the active Sun-like star CoRoT-7.This technique treats intrinsic stellar variability as correlated noise, using Gaussian process regression.I gave an introductory-level talk on Gaussian processes at the 2018 Sagan Summer School, which you can watch here.
Using exoplanet observations to place Earth into its astronomical context:Exoplanet discoveries are driving a new kind of Copernican revolution, prompting humanity to reflect on its place in the Cosmos. Recent observations show that planets are common, particularly planets with sizes similar to Earth's; but just as each one of us is unique, so is every Earth. The history of our own Earth shows that small changes in atmospheric properties can dramatically affect a planet's suitability for life. Placing Earth in this astronomical and geological context demonstrates that Earth is our only home, a fact that can inspire many to action.Simultaneously, astronomy inspires awe, which is shown to stimulate tolerance and catalyze collective action.
In 2019, I obtained a Certificate in Sustainability at Harvard's Extension School. The understanding I acquired of social and environmental issues on Earth has emboldened me to create opportunities for astronomers to weigh in on them. Last year, I organised a session: "Engaging the cosmic perspective on environmental and social issues" at NASA's Hubble Fellows Symposium (see my introductory slides here). I spoke at NASA headquarters on this topic in March 2020. Last September, on an academic visit in Sao Paulo, Brazil, I gave a seminar highlighting observations of the Amazon rainforest seen from space, to urge its protection (see my talk slides here).