Humboldt, Alexander von: Kosmos. Entwurf einer physischen Weltbeschreibung. Bd. 3. Stuttgart u. a., 1850.
Die letztere Abbildung giebt die Nomenclatur der einzelnen Regionen des, von so vielen Astronomen durchforschten Orions-Nebels. 67 (S. 337.) Delambre, Hist. de l'Astr. moderne T. II. p. 700. Cassini rechnete die Erscheinung dieses vierten Sternes ("aggiunta della quarta stella alle tre contigue") zu den Veränderungen, welche der Orions-Nebel in seiner Zeit erlitten habe. 68 (S. 338.) "It is remarkable that within the area of the trapezium no nebula exists. The brighter portion of the nebula immediately adjacent to the trapezium, forming the square front of the head, is shown with the 18-inch reflector broken up into masses, whose mottled and curdling light evidently indicates by a sort of granular texture its consisting of stars; and when examined under the great light of Lord Rosse's reflector or the exquisite defining power of the great achromatic at Cambridge, U. S., is evidently perceived to consist of clustering stars. There can therefore be little doubt as to the whole consisting of stars, too minute to be discerned individually even with the powerful aids, but which become visible as points of light when closely adjacent in the more crowded parts." (Outlines p. 609.) William C. Bond, der einen 23füßigen, mit einem 14zölligen Objectiv versehenen Refractor anwandte, sagt: "there is a great diminution of light in the interior of the Trapezium, but no suspicion of a star" (Mem. of the Amer. Acad., new Series Vol. III. p. 93). 69 (S. 338.) Philos. Transact. for the year 1811 Vol. CI. p. 324. 70 (S. 338.) "Such is the general blaze from that part of the sky", sagt der Capitän Jacob (Bombay Engineers) zu Punah, "that a person is immediately made aware of its having risen above the horizon, though he should not be at the time looking at the heavens, by the increase of general illumination of the atmosphere, resembling the effect of the young moon." Transact. of the Royal Soc. of Edinburgh Vol. XVI. 1849 Part 4. p. 445. 71 (S. 338.) Kosmos Bd. III. S. 251-254. 72 (S. 339.) Capreise § 70-90 Pl. IX, Outlines § 887 Pl. IV fig. 2. 73 (S. 339.) Kosmos Bd. II. S. 146. Die letztere Abbildung giebt die Nomenclatur der einzelnen Regionen des, von so vielen Astronomen durchforschten Orions-Nebels. 67 (S. 337.) Delambre, Hist. de l'Astr. moderne T. II. p. 700. Cassini rechnete die Erscheinung dieses vierten Sternes (»aggiunta della quarta stella alle tre contigue«) zu den Veränderungen, welche der Orions-Nebel in seiner Zeit erlitten habe. 68 (S. 338.) »It is remarkable that within the area of the trapezium no nebula exists. The brighter portion of the nebula immediately adjacent to the trapezium, forming the square front of the head, is shown with the 18–inch reflector broken up into masses, whose mottled and curdling light evidently indicates by a sort of granular texture its consisting of stars; and when examined under the great light of Lord Rosse's reflector or the exquisite defining power of the great achromatic at Cambridge, U. S., is evidently perceived to consist of clustering stars. There can therefore be little doubt as to the whole consisting of stars, too minute to be discerned individually even with the powerful aids, but which become visible as points of light when closely adjacent in the more crowded parts.« (Outlines p. 609.) William C. Bond, der einen 23füßigen, mit einem 14zölligen Objectiv versehenen Refractor anwandte, sagt: »there is a great diminution of light in the interior of the Trapezium, but no suspicion of a star« (Mem. of the Amer. Acad., new Series Vol. III. p. 93). 69 (S. 338.) Philos. Transact. for the year 1811 Vol. CI. p. 324. 70 (S. 338.) »Such is the general blaze from that part of the sky«, sagt der Capitän Jacob (Bombay Engineers) zu Punah, »that a person is immediately made aware of its having risen above the horizon, though he should not be at the time looking at the heavens, by the increase of general illumination of the atmosphere, resembling the effect of the young moon.« Transact. of the Royal Soc. of Edinburgh Vol. XVI. 1849 Part 4. p. 445. 71 (S. 338.) Kosmos Bd. III. S. 251–254. 72 (S. 339.) Capreise § 70–90 Pl. IX, Outlines § 887 Pl. IV fig. 2. 73 (S. 339.) Kosmos Bd. II. S. 146. <TEI> <text> <body> <div n="1"> <div n="2"> <div n="3"> <div n="4"> <div n="5"> <note xml:id="ftn423-text" prev="#ftn423" place="end" n="66"><pb facs="#f0371" n="366"/> Die letztere Abbildung giebt die Nomenclatur der einzelnen Regionen des, von so vielen Astronomen durchforschten Orions-Nebels.</note> <note xml:id="ftn424-text" prev="#ftn424" place="end" n="67"> (S. 337.) <hi rendition="#g">Delambre, Hist. de l'Astr. moderne</hi> T. II. p. 700. Cassini rechnete die Erscheinung dieses vierten Sternes (»aggiunta della quarta stella alle tre contigue«) zu den Veränderungen, welche der Orions-Nebel in seiner Zeit erlitten habe.</note> <note xml:id="ftn425-text" prev="#ftn425" place="end" n="68"> (S. 338.) »It is remarkable that within the area of the trapezium no nebula exists. The brighter portion of the nebula immediately adjacent to the trapezium, forming the square front of the head, is shown with the 18–inch reflector broken up into masses, whose mottled and curdling light evidently indicates by a sort of granular texture its consisting of stars; and when examined under the great light of Lord Rosse's reflector or the exquisite defining power of the great achromatic at Cambridge, U. S., is evidently perceived to consist of clustering stars. There can therefore be little doubt as to the whole consisting of stars, too minute to be discerned individually even with the powerful aids, but which become visible as points of light when closely adjacent in the more crowded parts.« <hi rendition="#g">(Outlines</hi> p. 609.) William C. Bond, der einen 23füßigen, mit einem 14zölligen Objectiv versehenen Refractor anwandte, sagt: »there is a great diminution of light in the interior of the Trapezium, but no suspicion of a star« <hi rendition="#g">(Mem. of the Amer. Acad.,</hi> new Series Vol. III. p. 93).</note> <note xml:id="ftn426-text" prev="#ftn426" place="end" n="69"> (S. 338.) <hi rendition="#g">Philos. Transact.</hi> for the year 1811 Vol. CI. p. 324.</note> <note xml:id="ftn427-text" prev="#ftn427" place="end" n="70"> (S. 338.) »Such is the general blaze from that part of the sky«, sagt der Capitän <hi rendition="#g">Jacob</hi> (Bombay Engineers) zu Punah, »that a person is immediately made aware of its having risen above the horizon, though he should not be at the time looking at the heavens, by the increase of general illumination of the atmosphere, resembling the effect of the young moon.« <hi rendition="#g">Transact. of the Royal Soc. of Edinburgh</hi> Vol. XVI. 1849 Part 4. p. 445.</note> <note xml:id="ftn428-text" prev="#ftn428" place="end" n="71"> (S. 338.) <hi rendition="#g">Kosmos</hi> Bd. III. S. 251–254.</note> <note xml:id="ftn429-text" prev="#ftn429" place="end" n="72"> (S. 339.) <hi rendition="#g">Capreise</hi> § 70–90 Pl. IX, <hi rendition="#g">Outlines</hi> § 887 Pl. IV fig. 2.</note> <note xml:id="ftn430-text" prev="#ftn430" place="end" n="73"> (S. 339.) <hi rendition="#g">Kosmos</hi> Bd. II. S. 146.</note> </div> </div> </div> </div> </div> </body> </text> </TEI> [366/0371]
⁶⁶ Die letztere Abbildung giebt die Nomenclatur der einzelnen Regionen des, von so vielen Astronomen durchforschten Orions-Nebels.
⁶⁷ (S. 337.) Delambre, Hist. de l'Astr. moderne T. II. p. 700. Cassini rechnete die Erscheinung dieses vierten Sternes (»aggiunta della quarta stella alle tre contigue«) zu den Veränderungen, welche der Orions-Nebel in seiner Zeit erlitten habe.
⁶⁸ (S. 338.) »It is remarkable that within the area of the trapezium no nebula exists. The brighter portion of the nebula immediately adjacent to the trapezium, forming the square front of the head, is shown with the 18–inch reflector broken up into masses, whose mottled and curdling light evidently indicates by a sort of granular texture its consisting of stars; and when examined under the great light of Lord Rosse's reflector or the exquisite defining power of the great achromatic at Cambridge, U. S., is evidently perceived to consist of clustering stars. There can therefore be little doubt as to the whole consisting of stars, too minute to be discerned individually even with the powerful aids, but which become visible as points of light when closely adjacent in the more crowded parts.« (Outlines p. 609.) William C. Bond, der einen 23füßigen, mit einem 14zölligen Objectiv versehenen Refractor anwandte, sagt: »there is a great diminution of light in the interior of the Trapezium, but no suspicion of a star« (Mem. of the Amer. Acad., new Series Vol. III. p. 93).
⁶⁹ (S. 338.) Philos. Transact. for the year 1811 Vol. CI. p. 324.
⁷⁰ (S. 338.) »Such is the general blaze from that part of the sky«, sagt der Capitän Jacob (Bombay Engineers) zu Punah, »that a person is immediately made aware of its having risen above the horizon, though he should not be at the time looking at the heavens, by the increase of general illumination of the atmosphere, resembling the effect of the young moon.« Transact. of the Royal Soc. of Edinburgh Vol. XVI. 1849 Part 4. p. 445.
⁷¹ (S. 338.) Kosmos Bd. III. S. 251–254.
⁷² (S. 339.) Capreise § 70–90 Pl. IX, Outlines § 887 Pl. IV fig. 2.
⁷³ (S. 339.) Kosmos Bd. II. S. 146.
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| Zitationshilfe: | Humboldt, Alexander von: Kosmos. Entwurf einer physischen Weltbeschreibung. Bd. 3. Stuttgart u. a., 1850, S. 366. In: Deutsches Textarchiv <https://www.deutschestextarchiv.de/humboldt_kosmos03_1850/371>, abgerufen am 25.11.2024. |
