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  1. The Astronomy and Astrophysics Review
  2. The Astronomy and Astrophysics Review : Volume 20
  3. The Astronomy and Astrophysics Review : Volume 20, Issue 1, October 2012
  4. Our astrochemical heritage
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The Astronomy and Astrophysics Review : Volume 24
The Astronomy and Astrophysics Review : Volume 23
The Astronomy and Astrophysics Review : Volume 22
The Astronomy and Astrophysics Review : Volume 21
The Astronomy and Astrophysics Review : Volume 20
The Astronomy and Astrophysics Review : Volume 20, Issue 1, October 2012
Interferometric observations of rapidly rotating stars
Multiple populations in globular clusters : Lessons learned from the Milky Way globular clusters
Imaging the heart of astrophysical objects with optical long-baseline interferometry
Turbulent molecular clouds
Clusters of galaxies: observational properties of the diffuse radio emission
Our astrochemical heritage
Circumstellar disks and planets : Science cases for next-generation optical/infrared long-baseline interferometers
Supernova remnants: the X-ray perspective
The Astronomy and Astrophysics Review : Volume 19
The Astronomy and Astrophysics Review : Volume 18
The Astronomy and Astrophysics Review : Volume 17
The Astronomy and Astrophysics Review : Volume 16
The Astronomy and Astrophysics Review : Volume 15
The Astronomy and Astrophysics Review : Volume 14
The Astronomy and Astrophysics Review : Volume 13
The Astronomy and Astrophysics Review : Volume 12
The Astronomy and Astrophysics Review : Volume 11
The Astronomy and Astrophysics Review : Volume 10
The Astronomy and Astrophysics Review : Volume 9
The Astronomy and Astrophysics Review : Volume 8

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Our astrochemical heritage

Content Provider Springer Nature Link
Author Caselli, Paola Ceccarelli, Cecilia
Copyright Year 2012
Abstract Our Sun and planetary system were born about 4.5 billion years ago. How did this happen, and what is the nature of our heritage from these early times? This review tries to address these questions from an astrochemical point of view. On the one hand, we have some crucial information from meteorites, comets and other small bodies of the Solar System. On the other hand, we have the results of studies on the formation process of Sun-like stars in our Galaxy. These results tell us that Sun-like stars form in dense regions of molecular clouds and that three major steps are involved before the planet-formation period. They are represented by the prestellar core, protostellar envelope and protoplanetary disk phases. Simultaneously with the evolution from one phase to the other, the chemical composition gains increasing complexity.In this review, we first present the information on the chemical composition of meteorites, comets and other small bodies of the Solar System, which is potentially linked to the first phases of the Solar System’s formation. Then we describe the observed chemical composition in the prestellar core, protostellar envelope and protoplanetary-disk phases, including the processes that lead to them. Finally, we draw together pieces from the different objects and phases to understand whether and how much we inherited chemically from the time of the Sun’s birth.
Starting Page 1
Ending Page 68
Page Count 68
File Format PDF
ISSN 09354956
Journal The Astronomy and Astrophysics Review
Volume Number 20
Issue Number 1
e-ISSN 14320754
Language English
Publisher Springer-Verlag
Publisher Date 2012-10-31
Publisher Place Berlin, Heidelberg
Access Restriction One Nation One Subscription (ONOS)
Subject Keyword Astrochemistry ISM: clouds Stars: formation Protoplanetary disks Comets: general Meteorites, meteors, meteoroids Astronomy, Astrophysics and Cosmology Astrophysics and Astroparticles Astronomy, Observations and Techniques Planetology Extraterrestrial Physics, Space Sciences
Content Type Text
Resource Type Article
Subject Astronomy and Astrophysics Space and Planetary Science
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