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Where Lies Space

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          This is the first article in a series on topics related to space, including rocketry, imagined settlements on other planets, and journeying to distant worlds.

          On the first day, we might like to think about what space is. Where does it lie?

[ The word ‘space’ in Physics, denotes a basic concept. It is the physical entity which is necessary for an object to have volume or for distances and locations to exist. It is the ‘room’ required for an object to exist. But this is not our concern here ].

           Of course, we all know the vast expanse of room beyond our Earth, in all directions, in which are hanging the stars, planets going around them, clouds of gas and dust, and huge re-occurring clusters of these things.. is what we think of as ‘space’.

And our earth is our home, a familiar, beloved place. At times beautiful and at times a little mundane. Space is on the outside.

But how far exactly? From an Earth-dweller’s perspective, how far above the ground do we have to travel, in order to enter Space?

         Well everyone can form his or her own concepts in this matter. The top of one’s local water tower is not it, and a comet beyond the planet Neptune, is definitely part of it.

         So what is the defining boundary?

~

A LIFE-SUPPORTING ENVIRONMENT

        For example, a person might think that the height above the ground, at which there begins to be no air, or too little of it, so that a person wouldn’t be able to breathe and therefore live in, is where space begins.

         But do we need to go up all the way to what is commonly thought of as ‘space’, to experience that?

          Human beings cannot reside above an altitude of about 5300 metres.

-that is, a human being cannot stay permanently or for an extended period of time (say a few days or weeks) normally and naturally, in such places. Even if they be on the surface of the Earth.

[ Here ‘normally’ means – without medical problems or serious physical distress, and while maintaining the routine level of physical activity.

‘Naturally’ means – without any artificial aid to survival such as supplemental oxygen or medicines.

Altitude (of a given place) of course means the height of that place above the ‘mean sea level’ ].

        The three highest human settlements in the world happen to be located at elevations of 5,000 to 5100 metres. (They include a town in the Andes mountains of Peru and a couple of villages in Tibbet).

[ Here, only permanent, round-the-year settlements serving as home to common people are being considered; so a research station manned by scientists or an expeditionary camp in the Himalayas would not count ].   

It may be added that on the website mounteverest.info, Mr. Graham Hoyland, who is himself a mountaineer, writes ‘humans have survived for two years at 5950 metres, which is the highest recorded permanently tolerable altitude.’

         With adequate rest intervals, a healthy and very fit person could climb to a height of even 6100 metres (which is a little more than the height of Mt. Kilimanjaro) without an oxygen canister, and breathe normally there at rest.  

          But he would not be able to stay there permanently, or even for more than a day or two (going to sleep becomes very difficult or impossible; and the person may wake up in distress shortly within dozing off. This is due to the scarcity of oxygen; though initially, at rest, there may be no difficulty in breathing).

Food would not be digested properly. And he would probably be seriously out of breath if he attempted any substantial physical exertion.

*   

This is slightly divergent from the topic, but we will continue for just a while.

-Depending on his individual tolerance of high altitudes and at what rate he has made the ascent – the person may also develop Acute Altitude Sickness, the mildest and most common form of which is Acute Mountain Sickness. AMS is characterized by a set of symptoms including headache and possibly : lethargy, nausea, dizziness, shortness of breath, disturbed sleep, and in severe cases impaired mental functions/confusion. AMS occurs 6 to 48 hours after the altitude exposure begins. And depending upon certain factors, it may resolve on its own or worsen.

In severe cases of Acute Altitude Sickness, the person may develop pulmonary edema or cerebral edema (aka HAPE and HACE).. i.e. the accumulation of excess fluid in these organs. Acute Altitude Sickness can be fatal, but is so in less than 1% of all cases.

*   

                   However, this being an affair of Biology, there are exceptions, departures from the pattern too.

                    Men in their prime, including trekkers and natives of mountainous regions have been known to die of Acute Mountain Sickness after ascending to elevations of 4,000 metres. (Although this author didn’t find out whether they happened to have a relevant – perhaps undiscovered – pre-existing medical condition).

                    So there are considerable differences even among healthy individuals of the same age group in respect of their ability to withstand low oxygen concentrations.

     Interestingly, the physical troubles do not start with the difficulty in breathing itself, but with the effects of less quantity of oxygen in the air inhaled. Mostly headache.

     The cause of all of this is basically the lesser mass of air – including the lesser mass of oxygen – that a person is inhaling in each breath, as he/she ascends from the sea level. Beyond a certain point, it becomes impossible for the human body to tolerate it or get habituated to it.

      The atmospheric pressure – which is an indicator of the density of air – at the altitude of about 5600 metres is half of what it is at Mean Sea Level. This is a little higher than the Base Camp for Mount Everest. At the elevation of Mount Everest, the highest point on the Earth’s surface, it is only one-third of that at sea level.

       What could be the reason behind the progressively lower density of the atmosphere at greater distances from the Earth’s centre ?

*

        One might wonder, at what altitude would a human be unable to breathe normally, with immediate effect and even at rest, despite any amount of attempted acclimatization, and therefore be unable to survive for more than a short while?

        That height, it seems, is around 9.37 kilometres.

        The air at this level is so rare (i.e. of such low density), and therefore the atmospheric pressure is so small, that the air present beforehand in one’s lungs would be at a much higher pressure, and therefore flow out of the lungs into the space outside.

          It would simply not be physically possible for a human being to expand his lungs and chest cavity by such an extent that the pressure inside them becomes a little less than that of the air outside, and thereby that air may flow into the lungs.

[This is the current understanding of this author, which might not be completely accurate. He hasn’t done substantial thinking or study on this].   

          To survive at this height and beyond, any human being, no matter how good his physical condition, would need to breathe artificial oxygen. This needs to be ‘100% oxygen’.

(Can the reader put this in perspective, for example placing it besides the height at which a passenger aeroplane flies)?

*

           And from about 15.6 kilometres (~50,000 feet), the atmosphere is so thin that ‘the lungs cannot be inflated even using oxygen, necessitating a spacesuit’ or pressure-suit.

(A reader might recall that this is what Mr. Felix Baumgartner was dressed in, when he had jumped off a Helium balloon from an altitude of 39 kilometres in 2012).

           We might look at one other such threshold before moving on – at the height of 18 to 19 kilometres from the ground, the atmospheric pressure is so low (0.06 atmospheres) that the boiling point of water is the same as the normal temperature of the human body.

What this means is, if a human were present in such a region, exposed, then the water present in large amounts in his body tissues would begin to boil; the blood, mucus and other body fluids would start boiling. The person would rapidly lose consciousness and die if not restored to ‘normal’ ambient pressure within 90 seconds.

       -So even inhaling oxygen at high pressure would not save his life.

This level is called the Armstrong Limit. (Not after Neil Armstrong, but after Harry George Armstrong, an officer in the American air force, a doctor, and a pioneer in aviation medicine and aerospace medicine. He saw service till 1957 and authored many papers).

Of course, as we have seen, astronauts do space-walks at much greater heights and perform repairs to the International Space Station, because again, they are wearing space-suits which – among their other interesting and necessary provisions – are also internally pressurized to guard against this very problem.

*

       Continuing, above the elevation of 8,000 metres (the peaks of fourteen mountains in the world are this high, the highest being Mount Everest at 8849 m), not even expert mountaineers could survive for more than a few days. – Unless they are consuming supplemental oxygen. Without breathing in from their oxygen cylinders, after sometime, they would be steadily deteriorating.

There may be the permanent loss of some brain cells, too.

      Acclimatization beyond 8,000 metres is simply not possible.

[ It is for some reason that the areas of mountains above 8,000 metres have been called  – somewhat unceremoniously – the ‘death zone’ ].

By the way, the cold at these altitudes, the reduced levels of humidity and to some extent the elevated levels of ultraviolet rays in the sunlight – all make respiratory function and general human well-being, difficult.

     But the views are divine.

      If only the person makes use of some technology and knowledge to prevent any harm to himself.

       It certainly doesn’t look abnormal, looks quite natural, from these heights.

*

    If the reader is interested.. if they are properly acclimatized and were using supplemental oxygen during the climb, then an average Everest mountaineer can survive without oxygen on the top for about 12 hours. -Perhaps a little more.

The aforementioned Mr. Graham Hoyland, once took off his oxygen mask upon reaching the summit and remained so for half an hour, and he ‘was okay’.

The record in this respect is 21 hours by Babu Chiri Sherpa (of Nepal) who in May 1999 stayed at the summit for that duration.

One might think, if a person from around the sea level is air-dropped directly on to the summit of Mount Everest, what the effect upon him would be.

As a matter of fact, he would very soon ‘lose consciousness and die within minutes’.

*

      So, to sum up, should we define the boundary of Space by the criterion of whether at a certain distance from the surface of the Earth, there is sufficient air to sustain human life normally?

(And permanently).

       If we do, then Space would begin from a height of about 5500 metres to 6000 metres from the sea level. And most of us would not feel like calling this ‘Space’ !

     For one, it does not look like Space – what layman’s conception we have of it. It is blue skies, white clouds and terra firma all around.

Besides, there are many places on Earth, the slopes and peaks of the highest mountains, which exceed this height and where one can still stand very much on the ground.

      [Can the region of space just above the peak of the highest mountain of the Earth be called Space?

     I suppose it is a subjective view. A way of thinking.

     There does not seem to be any natural justification or necessity to call this Space].

     The same can be said of the thresholds of 9.37 kilometres and 15.6 kilometres (approximately) of altitude, outlined above.

     It also seems to this author that in a way, these lines are too human body-centric.

     Could the criterion be more ‘natural’ i.e. Physics- or Earth Sciences-based?

~

SKY OR SPACE ?

    Does one feel that space begins where the sky begins to look black? —-Rather than the blue or other hues it has when seen from near the ground.

     This would be a visual or ‘impression’-related conception of Space.

I find it naturally appealing.

  There are certain heights above the Earth where around and above oneself, the surroundings appear black – except if one is looking directly at the sun – and stars are visible even during the day (‘day’ at such locations simply means ‘the duration of time in which one happens to be over the half of the planet which is facing the sun’).

     One could simply say that this is the height above the ground beyond which there is no sky, but the open regions of Space.

     From this altitude onwards, the background or the empty parts of one’s field of view is black.

Though we must be aware that in technological activities like space-faring, and the various technical calculations and considerations that go into it, as well as in basic sciences like astrophysics, definitions like the one above may not find much application.

*

                   Before coming to what this height is, we may quickly examine why this change in colour happens.

                   We see the sky as blue.

(And containing some other colours, at some other times).

                   But why should it be so?

                   Has it occurred to us to that question may arise, why we should see any colour or light at all, when we are facing away from the sun and looking above the ground?

*

                   In a part of the scene in front of us, we see a given colour, because light of a particular range of wavelengths – which is specific for that colour – is coming from that part of the scene and striking our eyes.

Each specific range of wavelengths (in the visual segment of the spectrum of electromagnetic radiations) produces the effect of ‘seeing’ a particular colour, in human beings (and some other creatures too).

[ Electromagnetic waves outside of the ‘visual range’ that is specific for human beings, do not produce the sensation of vision or colours in human beings ].

So, a particular range of wavelengths in the visual spectrum corresponds to a particular colour, and there are seven such wavelength ranges and their own respective colours.

*

                  So, when we see the sky as blue, it is a simple thought that light of blue colour must be coming from that part of the sky and entering our eyes.

[ When sometimes we see the colour of some parts of the sky as reddish or orange, it is because due to some reason (that are known), lights of those wavelengths – corresponding to those colours – are entering our eyes from those parts ].

                   Sunlight, as school books tell us, is white in colour – it is a mix of all the seven colours of the visible range. And indeed when we look at the sun itself, we see it as white (NEVER LOOK AT THE SUN DIRECTLY i.e. STRAIGHT-ON, AT ANY TIME OF THE DAY. IT MAY CAUSE PERMANENT DAMAGE TO YOUR EYES). Although brilliant and dazzlingly so.

When we see the colour of an object as white, it is because light of all the seven colours are coming into our eyes from the object at the same time, and the resultant experience of that in our visual perception – how our eyes sense this mix of different wavelengths and how our brain interprets it – is what we call ‘white’.

                   And similarly, when we see the sky as black, for example on a moonless night, it is because no light is coming from the direction of the sky to our eyes in such times.

Because ‘black’ is the colour that is perceived as the effect of no waves of the visual range reaching our eyes. So actually, it is the absence of any colours. -From the physics point of view.

                  Space too appears black, unless one happens to be gazing at a body that is luminous, like a star, the Moon or a bright nebula.

So obviously, there is no light of any visible wavelength that comes from the ‘empty’ parts of our field of view, in space.

                   But has it occurred to the reader, why we should expect the sky to look blue from the ground. All of sunlight is made up of rays of light (or photons, as you wish) travelling parallel to one another. And sunlight, before/unless it has been reflected or redirected in any other way by any material on or near Earth, comes only from one direction.

So why is it that when we look up at the sky, in any given direction away from the sun, we see blue? Even if we have our back to the sun?

We should see no colour or light at all, because the perception of vision is produced only when light is entering our eyes. Light that passes us by, -on the sides, or is moving away from us, would not produce any sensation of vision in us.

So, we should see such parts of our field of view as black.

                   If we see a colour even when we are facing away from the sun, it must be because light of this colour is coming from that direction to us, and indeed from all directions above the ground .. on the sides and at all angles above the ground.

                    What could be the source of this light?

                   Is sunlight being reflected by the air molecules?

Then why would light coming from a single direction be reflected in all directions, seen from any and every point on the ground; and even from airplanes- below oneself? Is that because the air molecules are moving randomly in all directions, and also their atoms are spherical, and there are a very large number of them, so collectively they are reflecting incoming light in all directions. Some of the sunlight passes straight through the upper layers of the atmosphere, because of the large gaps between the gas molecules, to be reflected by the lower layers or reach the ground.

Turns out, that is not what happens. Because the sizes of the different types of molecules of air are much smaller compared to the wavelengths of light, and also because their numbers per unit volume of air is too little, air molecules do not reflect light to a significant extent. -Not enough for our eyes to see.

                   But is there nothing else that can act as the source of the blue light or redirect the blue part of the sunlight to people’s eyes. And what happens to the rest of the colours of light present in the incoming sunlight?

                   The truth is, it is air that is the source of the blue light reaching our eyes from every direction above the ground.

And this causes the field of view above the ground to look like.. well, like the ‘sky’. – A layer or sheet above us, coloured most of the times in blue, spreading up from the horizons in a very large and lightly curving manner.

It does not look limited, blocking our view, or limiting.

It is because of the uniform and all-pervasive manner in which air, at all heights and regions above the ground (till a certain limit), sends out mostly blue light in all directions.

                    But if it is not by reflection, then how?

                    Well, the optical phenomenon responsible for causing this appearance is Rayleigh Scattering. This is a particular type of Scattering of light which is done mostly by air molecules and a small portion by dust particles suspended in the air. 

                    In it, there is an interaction of the molecules of air (and in general – to a lesser extent – of any transparent material) with electromagnetic radiation (including light) that is incident upon it.

Rayleigh Scattering occurs only when the size of the particles of the medium in question, is smaller than a particular limit. – smaller than about 1/15th of the wavelength of the radiation.

*

                 The molecules are made up of atoms.

                  Normally in an atom, the positively charged nucleus is at the centre and the electrons – which are negatively charged – are present around it, in a symmetrical way, in their respective, fixed geometric regions of space called orbitals.

Since under normal conditions, in the atom as a whole, there is no net separation of positive and negative charges between any two opposite points on its boundaries, therefore the atom is said to have no dipole moment.

                    An electromagnetic wave is basically periodic changes (within a range of values) in the intensity of an electric and a magnetic field (oriented perpendicular to each other) which together make up the electromagnetic field. These changes are also called ‘oscillations’ of the field.

                    When an electromagnetic wave is incident upon these atoms, then the oscillating electric field of the wave – i.e. the rhythmically changing intensity of the electric field which pervades the space in which these atoms are present, –causes a force to act upon the electrons and the nucleus of the atom, because of course they are electrically charged. And because they are oppositely charged, the respective forces they experience due to the external electric field, are in opposite directions, and these forces cause them to be displaced a little in opposite directions. Thus, the atom becomes electrically polarized – an electric dipole is created.

[ NOTE : This author does not know if the nucleus too is actually displaced. It is order of magnitudes heavier than the electrons, while being only 7 or 8 times more charged than an electron, so its displacement i.e. oscillating motion might be negligible compared to the electrons’.

But even if only the electrons oscillate, i.e. are displaced a little away from the nucleus, an electric dipole would still be created, because of the non-balanced distribution of electric charge within the atom ].     

                   Now, if you remember, an electromagnetic wave essentially is made up of an electric and a magnetic field, such that at each given point within the field, the strength or intensity of the electric or magnetic field is varying regularly over time, repeatedly.

                   So the charged particles of the atom – the electrons and the nucleus – must also be experiencing forces upon themselves which are varying in strength periodically (a very small period) ; and therefore, the amount by which they are being excited or displaced is also varying in time. And therefore, the electric dipole moment created by their displacements must also be varying in magnitude periodically.

                   And here we come to the crux of this natural phenomenon.. according to the classical electromagnetic theory (Maxwell’s Equations), an accelerating charge generates electromagnetic waves. The oscillating electron is such a thing.

This oscillating electric dipole in turn creates its own electromagnetic waves. These waves are emitted by the atom in all directions, (–equally, in Rayleigh Scattering; in some other forms of Scattering, the intensity of emissions is not uniform in all directions).

What wavelength or mix of wavelengths the emitted radiation will have, is dependent upon what wavelength/s are present in the incident radiation, and the size and nature of the scattering particles.

                   So, in this way, air molecules receive sunlight and then re-emit, i.e. ‘scatter’ it in all directions.

Do you think a given air molecule, over a period of time, is scattering only the sunlight coming directly from the sun?

*

[ If the reader is interested, there is a succinct and good explanation of the mechanism of Rayleigh Scattering here :

https://physics.stackexchange.com/questions/235535/how-does-wavelength-affect-scattering-of-light-rays ].

*

                  Sunlight contains waves that are ordered in seven consecutive bands of wavelengths, corresponding to seven colours – the VIBGYOR that we know well.

                   But not all wavelengths of the received sunlight are re-emitted equally.

                    All wavelengths of light undergo scattering, indeed radiations of wavelengths above or below the visual range for human beings i.e. wavelengths other than those of ‘light’, also do, but the smaller wavelengths of radiation undergo scattering much more strongly.

[ ‘Strongly’ here means that the intensity or share of energy, in the overall scattered radiation, is much more for smaller wavelengths, than what would have been by arithmetic proportions within the incoming spectrum ].

                   Now if we look at the pattern of the wavelengths in sunlight, (we may

recall the short-form VIBGYOR from school), we see that blue light has a short range of wavelengths.

                   Well, violet and indigo have even shorter wavelengths, but the colour of the sky is almost never violet. This is for two reasons.

The proportion of violet light present in sunlight is much smaller than that of blue. That is the very nature of the overall radiation emitted from the sun. In fact, the amount of green light is the most in sunlight.

 Secondly, the human eye is more sensitive to light of blue colour than violet or indigo.

                    About one-quarter of the incoming sunlight is scattered in this way.

(The rest passes through to the ground; a little is absorbed by the air, which causes it to become warm).

[ Actually, as may be guessed, the blue light that reaches us on the ground is not coming from having been scattered at one place only. It has been scattered and re-scattered numerous times by the time it has reached our eyes ].

The question may also arise, if air causes sunlight to be scattered into predominantly blue colour and reach our eyes, such that a mass or sample of air in front of a person, sends blue light toward him (and in all other directions) when the sun is not in line with the two, then how can we see a highrise building say two kilometres from us? Should the intervening mass of air not make the whole scene appear blue?

And how about a far away hill?.

*

                  Unlike our Moon, the rocky planets around the Sun do have atmospheres (except Mercury, whose is extremely thin).

                   So could we surmise that the skies on these planets are blue, too? Because it is this colour of light in the solar spectrum (i.e. the visible part of it) that has the smallest wavelength, and therefore is scattered most strongly?

But in the atmosphere of Mars, the proportion of dust particles is much more than in that of Earth.

And the density of gases is less than one percent of that of Earth’s.

Further, the composition of Mars’ atmosphere, -the predominant gas which constitutes it, is different from that of Earth’s. (95% of it is carbon dioxide). Therefore due to the different constituents of the Mars’ atmosphere, sunlight is scattered in a different way in the sky of Mars.

The colour of the sky on Mars is not blue, but reddish for most of the day. When the sun is near the horizon, that is around the time of sunrise or sunset, the sky takes on a pale bluish hue.

The sun – being almost double the distance from Mars as from Earth – looks quite a bit smaller than from Earth. It is also dimmer. (-despite the tenuous atmosphere).                       

*

              Now, we know that Earth’s gravity – the force of its attraction towards its centre – is strongest at its surface (i.e. the surface of its solid/liquid part), and decreases in strength with the increase in distance from the surface. 

            So naturally, most of the air around the Earth is present in the lower altitudes, and not evenly distributed through the extent of the atmosphere. In other words, the density of the atmosphere decreases steadily with the increase in height from the ground.

In fact, the decrease is almost exponential i.e. very steep, in the upper reaches.

              Away from the Earth, outwards, lies the near vacuum of space. The atmosphere gradually becomes fainter and fainter until it becomes non-existent; the extremely thin mass of atoms spread wide apart, merges into space.

*

              It would seem sensible to assume that since the blue colour of our general field of view, as we look up from the surface of the Earth, is caused by the Scattering of sunlight by air molecules, therefore the heights above the Earth where there is no more air, the surroundings would look black.

              But do the open, unobstructed parts of one’s field of view appear black only from where the atmosphere ends? Or does the scattering effect become sufficiently weak at a certain height above the Earth – because the air in those regions is sufficiently scanty – such that it creates the appearance of blackness – at least to the sensitivity of the human eye – even before the atmosphere ends completely? (And as common sense would suggest, on the way to becoming completely black, the blue sky would gradually assume a darker and darker shade of blue).

              If we return to the Mount Everest for a moment, it is mentioned that the air pressure here is only one-third of what it is at sea level.

              So the amount of air per unit volume of space here must be one-third of that in the plains. And so the Rayleigh Scattering effect must be much less.

               And this arrangement of nature does have the expression that one would expect it to have. From the summit of Mt. Everest, the sky above does look a considerably darker shade of blue, than the parts of the sky below.

In fact, one can observe the beautiful pattern of the sky becoming darker and darker, as one raises one’s gaze from the horizon below, toward the zenith.

                The same effect can be observed from an airplane if one bends his neck a little to look upward. The sky above is of darker shades of blue than below. A passenger plane of today flies at an altitude of about 10 to 13 kilometres (its ‘cruising’ height). 

(contd.) –

                 Long before the Earth’s atmosphere ceases to exist, the ‘sky’ or the open parts of one’s field of view becomes black.                   

                 The height from which the air begins to be so rare that the scattering effect is negligible, are the regions where during the day, if one is not directly looking at the sun, the sky around and above him is dark. If we wish, we may call this region ‘space’.

*

                   And what is this height above the ground?

                   It is about 80 kilometres.

                    And stars are seen scattered in it, even ‘during the day’.

*

                    But if one imagines space in this way, he needs to be aware of some other things.

                    For example, there is no atmosphere over the Moon. Even at ground level, gas molecules are practically absent. So, if on the surface of the Moon, a person were to look up, what would his view be like?

                    If blackness of the sky above a certain altitude from the surface of a celestial body is taken as the criterion for defining Space, then would Space begin at the same distance near all planets and moons? While many solid celestial bodies have an atmosphere around them, many others – like our Moon and Mercury – have very little or none to speak of. So there would be not be the effect of a coloured sky looking up even from the ground, on these bodies. The sky from the ground on such heavenly bodies appears black.

Furthermore, the density, composition and width of the atmosphere is different for different planets and moons. -which would all combine to make for different altitudes from which their respective skies would begin to appear black.

For example, Mars has an atmosphere whose pressure at ground level is less than one-hundredth of that of Earth’s. So Space, by this definition, would be much nearer.

*

              The sky is completely black looking up from the surface of the Moon or of Ceres, a dwarf planet (earlier considered an asteroid) between Mars and Jupiter. (Needless to say, -even during the day). So does that mean that Space starts just above the surface of the Moon or Ceres? Strangely enough, I feel that that notion makes sense.

Whether in terms of the appearance of the outward environs, the strength of the solar wind and cosmic radiation at the ground itself, or the extreme differences of temperature between day and night, -and between sun and shade, the conditions on the ground are indistinguishable from those in Outer Space.

The conditions from the point of view of the safety of human beings standing on the ground of these celestial bodies, are very similar, if not practically identical to those in Deep Space.

                The impression which is created in the mind of someone, is that a person standing on these celestial bodies is ‘exposed to Space’. And true to that idea, people who have visited these worlds or might some day, did or would have to wear spacesuits, just like an astronaut on a spacewalk outside her spaceship.

                All the moderating and softening influences of a healthy, substantial atmosphere are absent. The sun rays are stark and intense. Indeed, it begins to be harmful to human beings within a short period of time.

~

VIEW OF THE EARTH

                  Some people could think of ‘space’ as the regions above the Earth, from where if a person were to look ‘down’, (i.e. toward the Earth), she could get a sense of the roundness of the Earth.

-That is, the heights from where a sufficiently large portion of the Earth is visible such that it is seen to have a curved outline.

                   Or that space begins in the region from where one is able to see the whole of the Earth. -Its complete round figure.

                  -Or where, still farther away – in the scene in front of oneself, the Earth is only a modest, minor object, and most of what one sees is the empty expanse of space with stars dotted in.

                   This is a subjective thought of space.

                   Children unconsciously, and many other people in their common moods, may think of space in this way.

(Though children may often have a more advanced and nuanced understanding too).

                   These definitions are predicated upon simply the distance of a location from Earth.

                   Is there, can there be a sharp boundary or cut-off point in such a concept of Space?

                  Technically, it seems there can be.

*

                  The height beginning from which the curvature of the Earth becomes visible is about 10.6 kilometres above the sea level. (Provided that one’s angle of view is at least 60 degrees, and of course the horizon needs to be almost free of cloud).

However, just like the very first moments of the appearance of daylight at the end of night, are almost imperceptible and go unnoticed unless we were particularly trying to sense it, – indeed if we happen to be waking at the time, we are not even sure that day has just begun; we usually realise only after the first few minutes – similarly at the above mentioned altitude (which is a little less than 35,000 feet), the Earth’s curvature as evinced by the outline of the horizon, is very slight. And barely perceptible.

Only people with the most acute eyesight and making the best conscious effort would be able to detect it.

                      Below is the view from the window of a passenger airplane.

Curvature of Horizon
Curvature of the Horizon

(Credit : http://thulescientific.com/Lynch Curvature 2008.pdf)

                 The reader may judge for herself how pronounced the curvature is 🙂

Though some sources hold that for cruise altitudes of passenger jet-planes, this is more ‘an impression’ than a valid technical observation. Or a visual artifact generated by camera lenses.

Photographs containing the Earth’s surface taken from altitudes of say 30 or 50 kilometres, for example from a gas balloon, often depict the outline of the Earth as being more curved than what a human eye – say a pilot or astronaut – would see. That is, more curved than the actual. This is because a wide angle lens – often employed for such shots – especially produces this kind of a distortion (called ‘barrel distortion’). Even an ordinary camera lens can produce a similar kind of distortion if the angle of view happens to be wide enough. It can be avoided by framing the scene so as to have the horizon at the midline. -Or by using a ‘rectilinear lens’.

                   Even from the cabin of the Concorde (a passenger aeroplane developed jointly by a British and a French company, which flew from 1969 to 2003, at speeds of up to twice that of sound), whose cruise altitude was about 18 kilometres, only half of the passengers reported the horizon to appear to be curved. From the cockpit, the pilots – who had a far wider view than the passengers through their small windows – could appreciate the curvature better.

(Though even from the smaller passenger windows of a plane, a considerably wider view can be had simply by bringing one’s eyes very close to the glass).

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                  The altitude from which the curvature of the Earth is comfortably visible is around 21 kilometres, which is the height at which the American air force’s reconnaissance aircraft U2 operated. (It was a spy plane basically, whose job was to take photographs of things on the ground and intercept signals).

                   Here too, it is gentle.

                   We may compare this height to the height from which the sky begins to appear black during the day, which is about 80 kilometres.

                   The curvature of the Earth must have been more pronounced to the pilots of the SR71 Blackbird, another reconnaissance plane of the US Air Force, which flew at 25.9 kilometres while cruising.

                   High altitude balloons (filled with helium or hydrogen) fly at an upper range of about 37 to 53 kilometres (depending on how strong and technologically advanced a given balloon is).

(Hot air balloons can make for enjoyable rides, but they fly at much lower heights of about 1 kilometre. Though the highest one has gone is 20 kilometres). 

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                   The International Space Station goes around the Earth at an altitude of about 419 kilometres.

-With all its residents, its experimenting instruments and life support systems.

                    Even from the ISS only a small portion, and far from most of the hemisphere, can be seen.

Though let me say here that from photographs of the Earth and its environs that have been taken from the Station, it has seemed to me – from the overall impression created, the sense of the Earth being a spherical body, the black space above, the minute surface features visible on the globe – that this is ‘near space’. -Kind of a transition region between Earthly places and space proper.

Anyway, continuing –

At ground level, for a person of average height, the horizon is about 5 kilometres away. So looking in all directions i.e. in a 360o view, the width of the view would be 10 kilometres.

[ Sometimes this author likes articulating what is common sense/stating the obvious. So –

   This 10 kilometres is not the maximum distance to which one would see at one look or in one instant, but the maximum expanse or range of things an observer would be able to see from a given spot, if he turned his head around ].

                   From the tallest building in the world, one can see to a distance of more than a 100 kilometres.

                   From the tallest mountain peak in the world, about 335 kilometres.

                   There is a formula in trigonometry which calculates this.

                   From the International Space Station, the maximum distance on the Earth’s surface to which one can see, in any direction, is about 2,272 kilometres.

                   So the horizon to horizon distance is about 4,544 kilometres.

[This I guess is the straight line range. Accurately speaking, the horizon-to- horizon surface distance would be a little more.

Since the Earth’s surface is curved, I guess more of its surface features can be packed into the above straight line. Though further from the spot directly below, there would be more perspective distortion; perhaps some ‘loss of definition’ due to the curvature. Still, the amount of curvature at this altitude is mild, so I think in watching with one’s eyes, there is no possibility of missing out on any sizeable surface feature].

                   This is the patch of ground or ocean one would be able to see from the Station looking downwards with an unobstructed view.

(Needless to say, this is not the area of the Earth one gets to see from any one window of the ISS. But a crew-member doing a spacewalk who happens to be positioned on the Earth-facing surface of the Station shall get such a view. -Or a person sitting on a chair strung from the bottom surface).

                   How large a portion of the Earth’s surface does this constitute?

                   Well, the width of the continental United States (from the East coast to the West) is about 4,288 kilometres.

                   So, one would be able to see a region the size of America, and a little more.

View of the Earth from the International Space Station
View of North America from the International Space Station – three of the Great Lakes are seen

Employing the formula –  Distance (in km) = √(Height in metres + 13),

we would be able to determine the distance from the Earth at which most or all of it is visible.

Provided that we knew the diameter of the Earth, which is 12,742 km.

The ISS and the Earth

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                     As we rise above the Earth, the distance at which we begin to see the entire Earth is about nine-hundred-and-fifty to a thousand kilometres.

                     [ To be technically correct, in order to see literally the complete surface of one hemisphere, an observer would have to step back from the Earth to an infinite distance.                                       

                     If one were to travel to a distance of about a thousand kilometres, and gaze at the Earth, it may certainly appear to him that he has in his sight the whole Earth, or rather an entire half.

                     However, if a person takes notice of the significance of certain personal, daily life experiences, and also calls to mind certain photographs of the Earth taken from space, he would be able to extrapolate that from distances from a sphere that are comparable to the sphere’s size, the entire surface of the half that faces him, cannot be seen.

In fact, as with some such mathematical relationships studied in senior secondary school, the value in this case approaches very closely the full measure, but never reaches it.

So if we move away from Earth by a distance of say five times its width, we would be able to see almost or ‘practically’ the whole of a hemisphere, but still, a little less.

                      So, in something which may come as unexpected to many of us, the poles of the Earth are not actually visible from a geostationary orbit; they lie slightly beyond the horizon.. out of view. This is at a distance of nearly three times the Earth’s diameter.

Even from the Moon, about one-and-a-half percent of the Earth’s hemisphere is not actually visible to an observer. But of course this is so small that almost never would it have any practical or subjective significance].

(As a rule in optics – If the distance between the observer’s eyes is less than the diameter of the sphere, then only at infinite distance from the sphere, would it be possible to see the entire surface area of the hemisphere that faces the observer).

              Anyway, so what is meant, is not whether all of the Earth – that is literally all of a hemisphere, is visible – but that all of the circle of the Earth, is visible ‘in one view/frame’, in front of one’s eyes, without having to turn one’s head or move one’s eyes.

And for this, it has been assumed in this article that the Earth would need to occupy an area corresponding to about 120 degree in one’s field of view, no more. (What could be the total field of view of a human being?) And the distance from the surface of the Earth – corresponding to this angle – has been calculated.

                   This distance is about 986 kilometres.

                   The formula which helps us to determine it, is –

                   In the blue triangle below, according to a basic formula of trigonometry :

                    sin(60) = r/(r+h).

                    The altitude would be –

                    h = (r/sin60) – r = ~986 km.

Formula for the Curvature of the Earth

Now if we wanted to see the Earth as an object within a larger surrounding space, then would the calculation involve a greater angle in the above equation or lesser?

Well, we would have to move further from the Earth, so the angle spanned by the Earth in the observer’s field of view, would become less.

If we imagined the Earth as occupying a total angle of 90O in our field of view, then we would be watching the Earth from a distance of 2640 kilometres (from its surface).

And if the Earth occupied an angle of 60O, – whence it would constitute truly a minor object in the overall field of view – we would be viewing it from a distance of 6371 kilometres. 

(-All approximate values).

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[How far we can see from a given height above the surface, i.e. how much of the width of the Earth we can see at one look is given by the quantity – r/tan ].

(‘Ꝋ’ (theta) – being the angle marked in blue in the diagram above).

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                      In 1972, the spaceship Apollo 17 launched by NASA left its parking orbit around the Earth a few hours after lift-off and left for the Moon; as it was travelling toward the Moon, a crew member trained his camera rearward and through a port, took a photograph of the Earth.   

                       It was from a distance of 45,000 kilometres.

                      Here is the photo –       

View of the Earth from Space

      AS17-148-22727, from which the Blue Marble was cropped

        (Credit : NASA Johnson Space Centre)

I think the surrounding Space which the astronauts saw from here, i.e. their angle of view, was larger than the frame of this photograph. Unless the rim of the view port limited the range of vision.

                   The details would be better visible if one used a telescope or binocular.

                     As we can see, the Earth now covers less than less than half of the field of view, most of what one sees is the empty expanse of outer space and celestial bodies, and in this respect, we are finally in space.

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                     By the way, it may be mentioned that the above mission was the farthest human beings have travelled from Earth since then. Which probably gives some indication of the condition of enthusiasm for and importance accorded to such expeditions, in the minds of the governments of developed countries in the subsequent times.

Though it would be sensible to try and assess the overall benefits for humankind and also these particular countries, in spending massively on such persuasions. Yet some subjective as well as material arguments too could be made in favour.

                     Certainly, since then, a large number of probes for visual knowledge and also the collection of other kinds of information, have been sent to various celestial bodies of our solar system, and several space telescopes meant for different kinds of and depths of knowledge excavation, have been placed in orbit.

                     They tell us a lot about the processes taking place in distant heavenly bodies, their lives and nature. -Such as stars, galaxies and other remarkable objects. That gives us the ability to predict how they would behave in the future.

                     They even tell us in great depths about the very laws of nature!

These unmanned projects are very interesting, and yield information that can be both practically useful and valuable for more ideal purposes.

                     But on the whole, it would probably be better to try and explore at least a little more than what government agencies have done so far. The skills and experience acquired in such activities may have other far-reaching and multifarious benefits. -Including in unrelated fields.

This is especially in view of the fact that space projects (and it is true that generally, a mission with a human crew costs substantially more in time, effort and funds, and may involve risks to humans) actually cost much less than many other government undertakings like military campaigns, military productions, trying to gain strategic and geopolitical advantages.

(This author definitely believes that some kinds of military activities, even though tragic or expensive, are just and necessary. Simply because to not engage in them would be more harmful, if not now then someday).

                     If human beings – and all that is valuable and cherishable about us –  are to thrive forever, they would have to overcome future cosmological challenges like the heating up of-, and, later on, the enlargement of the Sun, perhaps things like Gamma Ray Bursts from other parts of the Galaxy, the eventual loss of the Earth’s magnetic field, and farther in the future, the extinction of the Sun itself; much farther still, the extinction of all the stars in the known universe, and after about 1034 years, perhaps even the degeneration of the proton.

For that, sooner or later, they would have to invest more in fundamental research, and also physical exploratory missions. They would have to develop capabilities in changing the course of nature at the level of stars and planets. And of course travel to other worlds, and make other worlds, and set up new homes there.

If we want our happiness, our loving relationships to survive, this would have to be done.

Because – as this author feels – wondrous things as the cosmos is filled with, human beings are still the most valuable things to exist. -that is known.

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Outer Space and Deep Space

                     Coming back to the topic, in the previous section, we talked about a voyage to the Moon. Regions of Space beyond the distance of the Moon, are called by many scientists Deep Space (with respect to the Earth).

Whereas the area outside and onwards of the Earth’s atmosphere, is called Outer Space.

From a general perspective, we may say Outer Space means all regions of space in between celestial bodies, such as stars, planets, nebulae and asteroids.

Continue ReadingPart 2/2

(Where Lies Space – 2)