• Aucun résultat trouvé

Fly me to the Moon

N/A
N/A
Protected

Academic year: 2021

Partager "Fly me to the Moon"

Copied!
2
0
0

Texte intégral

(1)

Publisher’s version / Version de l'éditeur:

Skygazing: Astronomy through the seasons, 2018-05-15

READ THESE TERMS AND CONDITIONS CAREFULLY BEFORE USING THIS WEBSITE. https://nrc-publications.canada.ca/eng/copyright

Vous avez des questions? Nous pouvons vous aider. Pour communiquer directement avec un auteur, consultez la

première page de la revue dans laquelle son article a été publié afin de trouver ses coordonnées. Si vous n’arrivez pas à les repérer, communiquez avec nous à [email protected].

Questions? Contact the NRC Publications Archive team at

[email protected]. If you wish to email the authors directly, please see the first page of the publication for their contact information.

NRC Publications Archive

Archives des publications du CNRC

This publication could be one of several versions: author’s original, accepted manuscript or the publisher’s version. / La version de cette publication peut être l’une des suivantes : la version prépublication de l’auteur, la version acceptée du manuscrit ou la version de l’éditeur.

For the publisher’s version, please access the DOI link below./ Pour consulter la version de l’éditeur, utilisez le lien DOI ci-dessous.

https://doi.org/10.4224/23003332

Access and use of this website and the material on it are subject to the Terms and Conditions set forth at

Fly me to the Moon

Tapping, Ken

https://publications-cnrc.canada.ca/fra/droits

L’accès à ce site Web et l’utilisation de son contenu sont assujettis aux conditions présentées dans le site LISEZ CES CONDITIONS ATTENTIVEMENT AVANT D’UTILISER CE SITE WEB.

NRC Publications Record / Notice d'Archives des publications de CNRC:

https://nrc-publications.canada.ca/eng/view/object/?id=35eb9d79-8dcb-4863-a535-564fddbeb31d https://publications-cnrc.canada.ca/fra/voir/objet/?id=35eb9d79-8dcb-4863-a535-564fddbeb31d

(2)

FLY ME TO THE MOON

Ken Tapping, 15thMay, 2018

This is the first time I have had the opportunity to squeeze one of my favourite jazz titles into an astronomy article. Considering the rigours of the journey and the hostile environment on the Moon, why would an astronomer like to go there?

Doing astronomy from the surface of the Earth is difficult. All the cosmic emissions have to get through the atmosphere on their way to our telescopes. Some emissions are totally blocked, some partially blocked and most suffer some form of distortion. In addition, there is the problem of people…us. Our way of life involves squirting enormous amounts of light in all directions. This makes the sky glow and hides faint astronomical objects. Fortunately, we are now realizing that in addition to light pollution costing us huge amounts of money in wasted energy, it is degrading our enjoyment of the natural world. However, our telescopes are driving to higher sensitivities, making them more vulnerable to light pollution. Luckily there are still some truly dark locations. Our radio telescopes are no better off. Manmade radio transmissions are everywhere. Our cars and even we ourselves carry at least one, maybe more active radio devices. WIFI is a fact of life and the demand for more radio services continues to grow. In addition to living with ground-based

interference, radio telescopes have to look past aircraft with their own internet connections and satellites providing a multiplicity of services. Up to 10,000 satellites will be launched in the next few years in order to provide worldwide access to 5G communication and data exchange services. At the moment there are no people and very few radio transmitters on the Moon, and no light pollution or sky glow. However, the Earth is still a problem. In the lunar sky it appears about four times the diameter of the Full Moon and shines three times brighter. The Earth is also enormously bright at radio wavelengths, because of our radio transmissions. There is a solution; we can put our telescopes on the other side of the Moon. Because

the Moon rotates once for every orbit, we never see the other side, and it never gets to see us, so we won’t have to deal with its optical and radio glare. However, there is still the Sun. The far side of the Moon is often, and wrongly, referred to as the “dark side”. The Sun shines there too. When the Moon is New, it is day on the far side. When it is Full, it is day on our side.

There are downsides. The Moon has no

atmosphere, so we will have to live in an airtight, radiation-screened base, probably underground, only going onto the surface as needed. There are huge temperature variations between lunar day and night, making it challenging to protect our mirrors and precision antennas from thermal distortion. Once we have beaten the challenges, our reward will be a better view of the universe than we have ever had before. So, why are we continuing to build our major new astronomical facilities on the surface of the Earth?

Until we have a manned base on the Moon, equipped with all the lab and workshop support we have here, lunar instruments will have to be

treated as space projects. Because it is hard to get a service engineer to a broken space or lunar telescope in a timely fashion, we will need to spend months or years striving for an extremely high level of reliability. With ground-based

telescopes, supported by workshops, lots of expert help and easy transportation, reliability is less of an issue, so instrumentation can be developed and deployed quickly. In addition, here on Earth, we can involve students in hands-on work on new instrumentation. One day, maybe in a couple of decades, we will be able to fly students to the Moon for their work, but not yet.

Venus is spectacular in the west after sunset. Jupiter rises at 9 pm, Saturn at 1 am and Mars at 2 am. The Moon will be New on the 15th.

Ken Tapping is an astronomer with the National Research Council's Dominion Radio Astrophysical Observatory, Penticton, BC, V2A 6J9.

Tel (250) 497-2300, Fax (250) 497-2355 E-mail: [email protected]

Références

Documents relatifs

(2013) Length-weight relationship and seasonal effects of the Summer Monsoon on condition factor of Terapon jarbua (Forsskål, 1775) from the wider Gulf of Aden including

Identification and detection of a novel point mutation in the Chitin Synthase gene of Culex pipiens associated with diflubenzuron resistance...

These depend on which actor controls the trait (the vector or the parasite) and, when there is manipulation, whether it is realised via infected hosts (to attract vectors) or

Brennan TP, Woods JO, Sedaghat AR, Siliciano JD, Siliciano RF, Wilke CO: Analysis of human immunodeficiency virus type 1 viremia and provirus in resting CD4+ T cells reveals a

The newly employed reactive magnetron co-sputtering technique has allowed us to enhance the absorption coefficient from the MLs owing to the high density of Si-ncs achieved and/or the

Market and communication schemes have taken a noticeable place in temples and some of them can be regarded as types of “mega-temples.” 2 This article describes the

Altogether, these results indicate that expression of the endogenous DRP1 protein is important for maintaining normal mitochondrial morphology in NHEK and that loss of this

sour rot symptoms in the field and in the laboratory (n = 5 bunches), ‘Post-harvest mild rot’ indicates fruit that were collected without rot symptoms but showed mild rot in