Skip to main content Accessibility help
×
Hostname: page-component-5c6d5d7d68-thh2z Total loading time: 0 Render date: 2024-08-08T20:18:49.117Z Has data issue: false hasContentIssue false

P - Palladium Pd to Promethium Pm

Published online by Cambridge University Press:  06 July 2010

Carlos Jaschek
Affiliation:
Université de Strasbourg
Mercedes Jaschek
Affiliation:
Observatoire de Strasbourg
Get access

Summary

This element was discovered in 1803 by W. Wollaston in London. The name alludes to the asteroid Pallas discovered in 1802 by Olbers. Pallas Athene is the name of the goddess of wisdom in Greek mythology.

lonization energy

PdI 8.3 eV, PdII 19.4 eV, PdIII 32.9 eV.

Absorption lines of PdI

The equivalent width of PdI 3405(2) in the sun is 0.036.

Behavior in non-normal stars

Pd was first discovered by Bidelman (1966) in one Ap star. PdII was found by Adelman (1974) in one Bp star of the Si-4200 subgroup and by Adelman et al. (1979) in another Ap star of the Cr-Eu subgroup.

Isotopes

Pd occurs in the form of six stable isotopes, namely Pd 102 104, 105, 106, 108 and 110, which occur in the solar system with frequencies 1%, 11%, 22%, 27%, 27% and 12% respectively. There exist also 15 short-lived isotopes and isomers. The longest lived is Pd107 with a half life of 7 × 106 years, which can be used for radioactive dating.

Origin

Pd 105, 106 and 108 are produced by both the r process and the s process. Pd110 is a pure r process product, Pd104 a pure s process product and Pd102 are pure p process product.

This element was discovered in 1669 by H. Brandt in Hamburg, Germany. The name phosphorus in Greek means bringer of light, which was also the name given to the planet Venus.

lonization energies

PI 10.5 eV, PII 19.7 eV, PIII 30.2 eV.

Absorption lines of PI

The equivalent width of PI 9796(2) in the sun is 0.012. According to Underhill (1977) it is present in an A 2Ia star.

Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 1995

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×