Javascript must be enabled to continue!
HOW DID HOLST CONDUCT ‘THE PLANETS’?
View through CrossRef
AbstractAny would-be conductor of The Planets needs first to consult Holst's own recordings of 1923 and 1926; then Imogen Holst's The Music of Gustav Holst (3rd edition, in particular Chapter XXVI), and her and Colin Matthews's contributions to the Collected Facsimile Edition, Volume III. Opinions vary as to how far the constraints of the early recording studio affected the composer's interpretation, so the recent discovery of a miniature score with Sir Henry Wood's annotations on the 1931 Prom performance, where Holst had no such inhibitions, is of unusual interest. Its positive attributes, side by side with Wood's merciless exposing of the difficulties encountered by the composer, are all there. Durations of three movements have been added in Holst's writing, and Wood's own timings shed further light although, sadly, muddied by errors and inconsistencies. But there is new food for thought regarding such aspects as the speed of Saturn and a reminder where the central melody of Jupiter is concerned.
Title: HOW DID HOLST CONDUCT ‘THE PLANETS’?
Description:
AbstractAny would-be conductor of The Planets needs first to consult Holst's own recordings of 1923 and 1926; then Imogen Holst's The Music of Gustav Holst (3rd edition, in particular Chapter XXVI), and her and Colin Matthews's contributions to the Collected Facsimile Edition, Volume III.
Opinions vary as to how far the constraints of the early recording studio affected the composer's interpretation, so the recent discovery of a miniature score with Sir Henry Wood's annotations on the 1931 Prom performance, where Holst had no such inhibitions, is of unusual interest.
Its positive attributes, side by side with Wood's merciless exposing of the difficulties encountered by the composer, are all there.
Durations of three movements have been added in Holst's writing, and Wood's own timings shed further light although, sadly, muddied by errors and inconsistencies.
But there is new food for thought regarding such aspects as the speed of Saturn and a reminder where the central melody of Jupiter is concerned.
Related Results
Interior dynamics of small-core and coreless exoplanets
Interior dynamics of small-core and coreless exoplanets
Since the first exoplanet detection in 1992, the study of exoplanets has received considerable attention. It is becoming apparent that the diversity of the general exoplanet popula...
Dynamics of giant planets in protoplanetary discs
Dynamics of giant planets in protoplanetary discs
New instruments such as the ALMA interferometer and SPHERE on VLT allowed to obtain a large number of high-resolution images of protoplanetary discs. In these images, substructures...
Multi-fluid hydrodynamical simulations of circumbinary planet formation via pebble accretion
Multi-fluid hydrodynamical simulations of circumbinary planet formation via pebble accretion
Context. Since the detection of the first known transiting circumbinary planet (CBP), Kepler-16b,by the Kepler mission, a total pf 14 CBPs have been detected, raising questions abo...
Holst’s Savitri Libretto
Holst’s Savitri Libretto
This article focuses on the libretto (the words) of Gustav Holst’s one-act opera Savitri (opus 25, 1908), which is based on a story told in the Mahabharata. The article introduces ...
Potential long-term habitable conditions on planets with primordial H-He atmospheres.
Potential long-term habitable conditions on planets with primordial H-He atmospheres.
<p><strong>Introduction:</strong> Planets that retain a primordial, H-He dominated atmosphere can have hydrogen act as a greenhouse gas: t...
Primordial Planets with an Admixture of Dark Matter Particles and Baryonic Matter
Primordial Planets with an Admixture of Dark Matter Particles and Baryonic Matter
It has been suggested that primordial planets could have formed in the early Universe and the missing baryons in the Universe could be explained by primordial free-floating planets...
Improving tidal modeling for rocky worlds
Improving tidal modeling for rocky worlds
<p>The high number of discovered close-in planets motivates the improvement of tidal modeling.Among the five thousand exoplanets discovered up to now, half of them ha...
Constraining planet formation with atmospheric observations from the V1298 Tau planet system
Constraining planet formation with atmospheric observations from the V1298 Tau planet system
<p>Theories of planet formation like core accretion mechanism&#160; have been successful over the years in explaining the formation gas giant planets and even...

