Top Banner
Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304 Nice Cedex4, France. Content : Introduction – few key questions. On the dynamical evolution of planets ? On the formation of planets ? On the possibility for life to develop around R The potential of GAIA.
13

Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

Jan 18, 2018

Download

Documents

Zoe Wilkinson

Planet detections : Discovery and understanding of Earth and Solar System : 5 bodies (Mercury, Venus, Mars, Jupiter, Saturn) at first sight distinguishable from the other stars because changing their place on the sky were discovered very early, Anaxagore ( , Eclipse mechanism), Aristote ( , Earth’s sphericity), Erastothènes ( , mesure of Earth’s diameter), Hipparque (-130, precession of Earth axis), Ptolémée (middle of 2snd century A.D., a model of Solar System), …, Copernic ( , Heliocentrisme), Kepler (1609, elliptical orbits). Discovery and understanding of Extrasolar planetary Systems : has started in with the discovery of planets around pulsars (2 cases apparently confirmed) and has continued with the discovery (since 1994) of giant planets around ‘normal stars’.
Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

Planets around evolved stars,few key questions that could be tackled with GAIA

Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304 Nice Cedex4, France.

Content : Introduction – few key questions. On the dynamical evolution of planets ? On the formation of planets ? On the possibility for life to develop around Red Giants ? The potential of GAIA.

Page 2: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.
Page 3: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

Planet detections :

Discovery and understanding of Earth and Solar System : 5 bodies (Mercury, Venus, Mars, Jupiter, Saturn) at first sight distinguishable from the other stars because changing their place on the sky were discovered very early, Anaxagore (-499-427, Eclipse mechanism), Aristote (-384-322, Earth’s sphericity), Erastothènes (-276-195, mesure of Earth’s diameter), Hipparque (-130, precession of Earth axis), Ptolémée (middle of 2snd century A.D., a model of Solar System), …, Copernic (1473 1543, Heliocentrisme), Kepler (1609, elliptical orbits).

Discovery and understanding of Extrasolar planetary Systems : has started in 1990-91 with the discovery of planets around pulsars (2 cases apparently confirmed) and has continued with the discovery (since 1994) of giant planets around ‘normal stars’.

Page 4: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

On the dynamical evolution of planets ?

1) Mass loss phenomenom and tidal dissipations between planets and the Red Giant star (Rasio et al. 1996) : no remaining planets inside 1 AU around a 1 solar massstar in evolution, Earth’s fate ?, other planets of our Solar System should survive.

2) Resonances in planetary systems like our own should lead to the ejection of planetsinside 5 AU.

Page 5: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

On the formation of planets ?

Since the discovery of planets around pulsar (Wolszczan and Frail 1992) with Msini of2.8 and 3.4 Earth’s masses and respectively at 0.47 and 0.36 AU, a second generationplanet formation is suggested around pulsars that may result from the merging of 2 dwarf starsfor instance (Livio et al 1992).

More generaly planets may form at different stages of the stellar evolution.

Page 6: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.
Page 7: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

Stingray nebula

In about 1000 years …

Page 8: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

On the possibility for life to develop around Red Giant stars ?

Terrestrial planets, around Reg Giants, in ‘Habitable zone’ offering possibility for life to develop can be discovered by GAIA (Lopez and Schneider 2002 submitted).

Page 9: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

Earth’formation-4.550 Gyrs

No trace of fossils

Résidus carbonés-3.850 Gyrs

700 Myrs at mostFor life occurence

-3.600 Gyrs

Oldest fossils known (cyanobacteries)-3.550 Gyrs

Heavy meterotic bombardementduring the first Gyr

Page 10: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

The potential of GAIA.

1) Red giants are bright and numerous but expected problems for planet detectionwith GAIA related to surface features linked to convection in the stellar atmosphere.

2) A problem probably relaxed for Sub-Giant stars around which searchingFor Earth’s like planets in habitable zones transiting long enough for life toDevelop is of strong interest.

3) A search of planets around White Dwarfs is very adapted to the potential of GAIA.A SIMBAD/CDS search show that nearly 400 WD of mv less than 15 exist. Type DO, DA,DB.

Page 11: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

In a sphere of 20 pc around the Sun (from AQ, Allen) :

Jupiter like planets produce well measurableReflex motion of the star, larger than 10 micro-arcsecs. Hundred of potential sources for such a detection.

A 10 Earth’s mass planet produces a reflex motionof the star of the order of 5 micro-arcsecs. Assuming theWD at 10 pc and of 0.6 solar mass and the planet at 1 AU.A few sources.

Page 12: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

Interferometry and circumstellar environments

Page 13: Planets around evolved stars, few key questions that could be tackled with GAIA Lopez Bruno Obs. De la Côte d’Azur, Dpt. Fresnel UMR 6528, BP 4229 06304.

Compagnons stars as a sub-product of this search of planets