mirror of
https://github.com/vale981/prosem-latex
synced 2025-03-04 09:11:41 -05:00
Update proseminar.tex
This commit is contained in:
vale981
GitHub
parent
35328b1390
commit
2d679b4e2d
1 changed files with 85 additions and 85 deletions
170
proseminar.tex
170
proseminar.tex
|
|
@ -46,7 +46,7 @@
|
|||
|
||||
{
|
||||
\usebackgroundtemplate{
|
||||
\includegraphics[width=\paperwidth]{material/peg_b.jpg}}
|
||||
\includegraphics[width=\paperwidth]{material/peg_b.jpg}}
|
||||
\begin{frame}[plain]
|
||||
\end{frame}
|
||||
}
|
||||
|
|
@ -76,28 +76,28 @@
|
|||
\end{itemize}
|
||||
\end{block}
|
||||
\end{frame}
|
||||
\begin{frame}
|
||||
\frametitle{A Working-Defintion}
|
||||
\begin{block}{IAU 2003 Recommendation}
|
||||
Planets $=$ Objects below 13 Jupiter masses.
|
||||
\end{block}
|
||||
\pause
|
||||
Another Proposal based on the solar system definition by Jean-Luc Margot:
|
||||
\begin{frame}
|
||||
\frametitle{A Working-Defintion}
|
||||
\begin{block}{IAU 2003 Recommendation}
|
||||
Planets $=$ Objects below 13 Jupiter masses.
|
||||
\end{block}
|
||||
\pause
|
||||
Another Proposal based on the solar system definition by Jean-Luc Margot:
|
||||
\begin{itemize}
|
||||
\item based on metric for the clearing of the orbit
|
||||
\begin{itemize}
|
||||
\item based on metric for the clearing of the orbit
|
||||
\begin{itemize}
|
||||
\item based on mass of start and planet, orbital period
|
||||
\end{itemize}
|
||||
\item classifies 99\% of the known planets
|
||||
\item based on mass of start and planet, orbital period
|
||||
\end{itemize}
|
||||
\end{frame}
|
||||
\item classifies 99\% of the known planets
|
||||
\end{itemize}
|
||||
\end{frame}
|
||||
|
||||
\section{Nomenclature and Units}
|
||||
\begin{frame}
|
||||
\begin{block}{Nomenclature}
|
||||
Name/Designation of Star + a Letter ('b', 'c', ...)
|
||||
\end{block}
|
||||
\pause
|
||||
Name/Designation of Star + a Letter ('b', 'c', ...)
|
||||
\end{block}
|
||||
\pause
|
||||
\begin{example}
|
||||
51 Pegasi b - first confirmed exoplanet around a normal star
|
||||
\end{example}
|
||||
|
|
@ -119,20 +119,20 @@
|
|||
% \frametitle{Some Orbital Parameters}
|
||||
% \begin{columns}[t]
|
||||
% \column{.7\textwidth}
|
||||
% \begin{itemize}
|
||||
% \item<1-> Period $P\;[\mathrm{days}]$
|
||||
% \item<2-> Semi Major Axis $a\;[\mathrm{au}]$
|
||||
% \item<3-> Eccentricity $\epsilon$
|
||||
% % \item<4->inclination $i\;[\degree]$ in respect to the reference plane
|
||||
% \end{itemize}
|
||||
% \begin{itemize}
|
||||
% \item<1-> Period $P\;[\mathrm{days}]$
|
||||
% \item<2-> Semi Major Axis $a\;[\mathrm{au}]$
|
||||
% \item<3-> Eccentricity $\epsilon$
|
||||
% % \item<4->inclination $i\;[\degree]$ in respect to the reference plane
|
||||
% \end{itemize}
|
||||
% \column{.3\textwidth}
|
||||
% \begin{block}{}<2->
|
||||
% \includegraphics[width=\textwidth]{material/el.png}
|
||||
% \end{block}
|
||||
% % \begin{block}{}<4->
|
||||
% % \includegraphics[width=\textwidth]{material/inc.png}
|
||||
% % \end{block}
|
||||
% \end{columns}
|
||||
% % \begin{block}{}<4->
|
||||
% % \includegraphics[width=\textwidth]{material/inc.png}
|
||||
% % \end{block}
|
||||
% \end{columns}
|
||||
% \end{frame}
|
||||
|
||||
\section{Challenges in Exoplanet Detection}
|
||||
|
|
@ -147,7 +147,7 @@
|
|||
\begin{example}
|
||||
Looking at the Solar System and 51 Pegasi ($d=\SI{50.9}{\lightyear}$):
|
||||
\begin{itemize}
|
||||
% \item Angular Separation of Eath: $\SI{0.06}{\arcsec}$
|
||||
% \item Angular Separation of Eath: $\SI{0.06}{\arcsec}$
|
||||
\item Angular Separation of 51 Pegasi b as seen from Earth: $\SI{0.003}{\arcsec}$
|
||||
\end{itemize}
|
||||
\pause
|
||||
|
|
@ -172,29 +172,29 @@
|
|||
\item stacking, interferometry and clever computer processing \pause
|
||||
\end{enumerate}
|
||||
|
||||
\end{frame}
|
||||
% \begin{frame}
|
||||
% \frametitle{Least Massive: Formalhaut b (2 Jup. Masses)}
|
||||
% \begin{figure}
|
||||
% \centering
|
||||
% \includegraphics[width=0.8\textwidth]{material/formb.jpg}
|
||||
% \caption{http://spacetelescope.org/images/html/heic0821a.html}
|
||||
% \end{figure}
|
||||
% \end{frame}
|
||||
\begin{frame}
|
||||
\frametitle{Coldest: Gliese 504 b ($\SI{240}{\celsius}$)}
|
||||
\begin{figure}
|
||||
\centering
|
||||
\figcite{0.45\textwidth}{material/glies.jpg}{http://www.nasa.gov/content/goddard/astronomers-image-lowest-mass-exoplanet-around-a-sun-like-star/index.html}
|
||||
\end{figure}
|
||||
\end{frame}
|
||||
\begin{frame}
|
||||
\frametitle{HR 8799 has 4 Planets}
|
||||
\begin{figure}
|
||||
\centering
|
||||
\inlineMovie{material/keck_exo.avi}{material/keck_ex_p.png}{.75\textheight}{https://www.manyworlds.space/index.php/tag/hr-8799/}
|
||||
\end{figure}
|
||||
\end{frame}
|
||||
\end{frame}
|
||||
% \begin{frame}
|
||||
% \frametitle{Least Massive: Formalhaut b (2 Jup. Masses)}
|
||||
% \begin{figure}
|
||||
% \centering
|
||||
% \includegraphics[width=0.8\textwidth]{material/formb.jpg}
|
||||
% \caption{http://spacetelescope.org/images/html/heic0821a.html}
|
||||
% \end{figure}
|
||||
% \end{frame}
|
||||
\begin{frame}
|
||||
\frametitle{Coldest: Gliese 504 b ($\SI{240}{\celsius}$)}
|
||||
\begin{figure}
|
||||
\centering
|
||||
\figcite{0.45\textwidth}{material/glies.jpg}{http://www.nasa.gov/content/goddard/astronomers-image-lowest-mass-exoplanet-around-a-sun-like-star/index.html}
|
||||
\end{figure}
|
||||
\end{frame}
|
||||
\begin{frame}
|
||||
\frametitle{HR 8799 has 4 Planets}
|
||||
\begin{figure}
|
||||
\centering
|
||||
\inlineMovie{material/keck_exo.avi}{material/keck_ex_p.png}{.75\textheight}{https://www.manyworlds.space/index.php/tag/hr-8799/}
|
||||
\end{figure}
|
||||
\end{frame}
|
||||
|
||||
\section{Historic Overview}
|
||||
% \subsection{Antique}
|
||||
|
|
@ -212,7 +212,7 @@
|
|||
% in which, colliding with one another and revolving in all manner
|
||||
% of ways, they begin to separate like to like.'' \hfill - \tiny{\textit{LEUCIPPUS, 480-420 B.C.}}
|
||||
% \end{quote}
|
||||
% \pause
|
||||
% \pause
|
||||
% \begin{quote}
|
||||
% ``There \alert{cannot be more worlds} than one world.'' \\ \hfill - \tiny{\textit{ARSITOTLE, 384–322 B.C.}}
|
||||
% \end{quote}
|
||||
|
|
@ -221,19 +221,19 @@
|
|||
\begin{frame}
|
||||
\begin{columns}[t]
|
||||
\column{0.7\textwidth}
|
||||
\begin{itemize}
|
||||
\item<1-> \small{\textit{KOPERNIKUS}} (1543) of course supported plurality
|
||||
\item<2-> \small{\textit{GIORDANO BRUNO}} (1548-1600) postulates spacial infinity
|
||||
\item<3-> \small{\textit{NEWTON}} (1548-1600) speculates about other solar systems
|
||||
\item<4-> \small{\textit{OTTO STRUVE}} (1952) proposes methods of exoplanet detection
|
||||
\end{itemize}
|
||||
\only<5>{$\longrightarrow$ In the following years: A lot of false-positives.}
|
||||
\column{0.3\textwidth}
|
||||
\only<1>{\figcite{\textwidth}{material/kop.jpg}{Icones, p. 36}}
|
||||
\only<2>{\figcite{\textwidth}{material/brun.jpg}{Neue Bibliothec}}
|
||||
\only<3>{\figcite{\textwidth}{material/newt.jpg}{National Portrait Gallery: NPG 2881}}
|
||||
\only<4->{\figcite{\textwidth}{material/struve.jpg}{US Post}}
|
||||
\end{columns}
|
||||
\begin{itemize}
|
||||
\item<1-> \small{\textit{KOPERNIKUS}} (1543) of course supported plurality
|
||||
\item<2-> \small{\textit{GIORDANO BRUNO}} (1548-1600) postulates spacial infinity
|
||||
\item<3-> \small{\textit{NEWTON}} (1548-1600) speculates about other solar systems
|
||||
\item<4-> \small{\textit{OTTO STRUVE}} (1952) proposes methods of exoplanet detection
|
||||
\end{itemize}
|
||||
\only<5>{$\longrightarrow$ In the following years: A lot of false-positives.}
|
||||
\column{0.3\textwidth}
|
||||
\only<1>{\figcite{\textwidth}{material/kop.jpg}{Icones, p. 36}}
|
||||
\only<2>{\figcite{\textwidth}{material/brun.jpg}{Neue Bibliothec}}
|
||||
\only<3>{\figcite{\textwidth}{material/newt.jpg}{National Portrait Gallery: NPG 2881}}
|
||||
\only<4->{\figcite{\textwidth}{material/struve.jpg}{US Post}}
|
||||
\end{columns}
|
||||
\end{frame}
|
||||
|
||||
\subsection{First Planets}
|
||||
|
|
@ -245,14 +245,14 @@
|
|||
\item<1-> 1992 - first radio pulsar timing planet
|
||||
\end{itemize}
|
||||
\action<2->{
|
||||
\begin{block}{1995 - First planet around 'real' star}
|
||||
\begin{itemize}
|
||||
\item discovered by Mayor, Queloz of University Geneva
|
||||
\item 4 day orbit, much closer than Mercury (Hot Jupiter), 1.9 Jupiter radii
|
||||
\end{itemize}
|
||||
\end{block}}
|
||||
\only<1>{\column{0.5\textwidth}\figcite{\textwidth}{material/puls.jpg}{https://photojournal.jpl.nasa.gov/catalog/PIA08042}}
|
||||
\only<2>{\column{0.5\textwidth}\figcite{\textwidth}{material/peg_b.jpg}{https://www.eso.org/public/russia/images/eso1517a/}}
|
||||
\begin{block}{1995 - First planet around 'real' star}
|
||||
\begin{itemize}
|
||||
\item discovered by Mayor, Queloz of University Geneva
|
||||
\item 4 day orbit, much closer than Mercury (Hot Jupiter), 1.9 Jupiter radii
|
||||
\end{itemize}
|
||||
\end{block}}
|
||||
\only<1>{\column{0.5\textwidth}\figcite{\textwidth}{material/puls.jpg}{https://photojournal.jpl.nasa.gov/catalog/PIA08042}}
|
||||
\only<2>{\column{0.5\textwidth}\figcite{\textwidth}{material/peg_b.jpg}{https://www.eso.org/public/russia/images/eso1517a/}}
|
||||
\end{columns}
|
||||
\end{frame}
|
||||
|
||||
|
|
@ -325,15 +325,15 @@
|
|||
\frametitle{Some Facts}
|
||||
\begin{columns}
|
||||
\column{.5\textwidth}
|
||||
\begin{itemize}
|
||||
\item exoplanets orbit all kinds of stars
|
||||
\item mass range: 0.02 to 5780 Earth Masses
|
||||
\item orbital period range: \SIrange{0.4}{3.2e5}{\day}
|
||||
\item semi major axis: \SIrange{0.00585}{113}{AU}
|
||||
\item furthest away: \SI{21190}{\lightyear}
|
||||
\end{itemize}
|
||||
\column{.5\textwidth}
|
||||
\figcite{\textwidth}{material/mass_sep.png}{http://exoplanets.org/plots}
|
||||
\begin{itemize}
|
||||
\item exoplanets orbit all kinds of stars
|
||||
\item mass range: 0.02 to 5780 Earth Masses
|
||||
\item orbital period range: \SIrange{0.4}{3.2e5}{\day}
|
||||
\item semi major axis: \SIrange{0.00585}{113}{AU}
|
||||
\item furthest away: \SI{21190}{\lightyear}
|
||||
\end{itemize}
|
||||
\column{.5\textwidth}
|
||||
\figcite{\textwidth}{material/mass_sep.png}{http://exoplanets.org/plots}
|
||||
\end{columns}
|
||||
\end{frame}
|
||||
|
||||
|
|
@ -389,7 +389,7 @@
|
|||
\figcite{\textwidth}{material/trap.jpg}{http://photojournal.jpl.nasa.gov/figures/PIA22093_fig1.jpg}
|
||||
\end{columns}
|
||||
\end{frame}
|
||||
|
||||
|
||||
{
|
||||
\usebackgroundtemplate{
|
||||
\includegraphics[width=\paperwidth]{material/trapbig.jpg}}
|
||||
|
|
@ -398,7 +398,7 @@
|
|||
\hfill \color{white} Thanks for your attention!
|
||||
|
||||
\btVFill
|
||||
|
||||
|
||||
\hfill\tiny\color{white}\url{https://www.spacetelescope.org/images/heic1713a/}\bigskip
|
||||
\end{frame}
|
||||
}
|
||||
|
|
@ -415,7 +415,7 @@
|
|||
\item \tiny{``A COMBINED VERY LARGE TELESCOPE AND GEMINI STUDY OF THE ATMOSPHERE
|
||||
OF THE DIRECTLY IMAGED PLANET, BETA PICTORIS b''} by Thayne Currie et al. \normalsize
|
||||
\item \tiny{``TEMPERATE EARTH-SIZED PLANETS TRANSITING A NEARBY
|
||||
ULTRACOOL DWARF STAR''} by
|
||||
ULTRACOOL DWARF STAR''} by
|
||||
Michaël Gillon et al. \normalsize
|
||||
\item \tiny{``NO LARGE POPULATION OF UNBOUND OR WIDE-ORBIT
|
||||
JUPITER-MASS PLANETS''} by Przemek Mróz et al. (Rogue Planets, not included in the talk) \normalsize
|
||||
|
|
|
|||
Loading…
Add table
Reference in a new issue